Supplement

Since the draft of this book was submitted, remarkable progress has been achieved in the field of the physics of emission-line stars. In this supplement, selected papers (published mostly in 2005 and 2006) are presented with some notes focusing into two topics: fine structure of emission-line forming regions (envelope, wind, and disk) and magnetic fields of early-type stars (February, 2007).

Structure of emission-line forming regions

With the advancement of optical and infrared interferometry and other so- phisticated observational techniques, dimensions and internal structure of the emission-line forming regions have been markedly unveiled recently and com- pared with theoretical models. Many types of interferometer systems have been developed and used for observations. They include Very Large Telescope Interferometer (VLTI, ESO), Infrared and Optical Telescope Array (IOTA, Mt. Hopkins), Navy Prototype Optical Interferometer (NPOI, US Naval Ob- servatory), Stellar Interferometer (Sydney University), and Center for High Angular Resolution Astronomy (CHARA Array, Mt. Wilson). Coronagraphic Imaging system with Adaptive Optics (CIAO, Subaru telescope) also yields high spatially resolved infrared images of stellar envelopes.

LBV and central stars of planetary nebulae Near-infrared observations with the VLTI have been carried out for Eta Cari- nae and the central star of planetary nebula CPD-56°8032 (Chesneau et al. 2006). Weigelt et al. (2006) measured different disk diameters of Eta Carinae in the continuum (4.3 mas), in HeI emission (6.5 mas), and in Bry emission (9.6 mas) in K band. Line emissions showed a larger diameter as compared to that in the continuum. Chesneau et al. (2005) also derived the sub-arcsecond structure of the Eta Carinae envelope in the narrow-band images at 3.74 and 4.05 urn. A butterfly-shaped dusty environment and a void around the cen- tral star were found. Through spectropolarimetric observations, Davies et al. (2005) found an aspheric and clumpy structure in the winds of LBVs, which is more apparent in stars of strong Hex emission.

503 504 Astrology of Emission-Line Stars

Be stars Stee et al. (2005) reviewed the methods and techniques of interferometric observations of hot star disks with application to Be and B[e] stars. In the optical region, Tycner et al. (2005, 2006) carried out narrow-band Hex interferometry using NPOI and found the intensity distribution in the en- velopes for y Cas and

mass loss until the disks vanish. Rivinius considered the lifecycles of classical Be stars, similar to the successive outburst scenario of Meilland. If not replenished by subsequent outbursts, the ring will finally dissipate and Be stars will become B star.

Mira variables Stratified structure of the circumstellar envelopes of Miras, such as the dif- ference in the radii of optical and radio photospheres and of inner dust shell, has been depicted by combined optical, infrared, and radio interferometers (Cotton et al. 2005, Whittkowiski and Boboltz 2005). Stellar diameters in the optical (Ireland and Scholz 2006, Ireland et al. 2005) and infrared (Millan- Gabet et al. 2005, Ohnaka et al. 2005) spectral regions revealed the marked dependence on the wavelength and pulsational phase of Mira stars, where we can see the effects of dust formation and pulsational shock propagation. Dy- namic models have been calculated and compared with observations (Ohnaka et al. 2006).

Herbig Ae/Be stars Highly spatially resolved observations of HESs in the optical and infrared spectral regions have been carried out mostly by three groups: VLTI Supplement 505

(Benisty et al. 2005, Preibisch et al. 2006), IOTA (Millan-Gabet et al. 2006, Monnier et al. 2005, 2006), and Subaru CIAO (Tamura and Fukagawa 2005, Fujiwara et al. 2006, Fukagawa et al. 2006, Honda et al. 2005, Lin et al. 2006, Okamoto et al. 2005). Far-UV long-slit spectrograph with the HST is also used to resolve the inner cavity of a disk (Grady et al. 2005). Complicated structure of circumstellar disks of dust or molecular gases, such as central cavity, asymmetric disk, spiral arms, etc., are elucidated, along with some relationship with the H(X emission intensity.

T Tau stars As in the case of HES, recent observations of the structure of accretion disks have been made in near- and mid-infrared spectral regions mainly at Mauna Kea (Subaru, Keck telescopes) and ESO (VLT). Particular attention has been paid to the imaging of the inner part of the disks. Akeson et al. (2005) con- firmed the existence of inner edge of dust disk using the Keck interferometer. Mayama et al. (2006) using the CIAO of Subaru telescope, and Duchene et al. (2005) combining Keck telescope II, resolveda complex circumstellar structure around the multiple system of T Tau. Quanz et al. (2006) and Millan-Gabet et al. (2006) observed the structure of optically thick accretion disk of FU Ori in mid-infrared band using the VLT interferometer.

Magnetic fields of early-type stars

It has long been supposed that early-type stars are lacking magnetic fields because of the absence of convection layers theoretically predicted. Recently, however, magnetic fields have been detected in early-type stars, particularly in Be and Herbig Ae/Be stars. Its significant effects on the structure and evolution of envelopes have become widely recognized.

Be stars Neiner and Hubert (2005) reviewed the indirect and direct methods of detec- tion based on oblique rotator models. Rotational modulation of spectral lines and X-ray fluxes provide a promising method. Smith and Balona (2006) and Smith et al. (2006) suggested the existence of strong magnetic fields on the surface of Be stars by analyzing short-term variabilities in B, V bands, line emissions, and X-ray fluxes. Several theoretical models for magnetic winds and disks are proposed, generally based on the oblique rotator scheme with dipole-like magnetic fields (Brown and Cassinelli 2005, Maheswaran 2005, Ud-Doula et al. 2005). Cassinelli and Neiner (2005) presented a broad discussion on the origin and dissipation of magnetic fields in Be stars. On the origin, two possible mech- anisms were proposed: one is the dynamo action in the convection core and 506 Astrology of Emission-Line Stars its transportation to the surface and envelope, and the other is that the fossil fields remained from the initial stage of star formation.

HES Detection and measurements of magnetic fields in HESs have been performed mainly at VLT, ESO, and at CFHT, Mauna Kea, using the spectropolarime- terse Hubrig et al. (2005, 2006) measured the magnetic fields for several HESs and found a large magnetic field of around 450 G for HD 139614 as the largest case among Herbig Ae stars. Yudin et al. (2006) detected Zeeman fea- tures in Call doublet and in metallic lines, whereas Yudin (2005) suggested the existence of localized magnetic fields generated during the evolution of circumstellar envelopes. Catala et al. (2007) observed the Herbig Ae starHD 190073 with the echelle spectropolarimetric device attached to the CFH Telescope, and de- tected the magnetic field in the photosphere of this star. Drouin et al. (2005) used both VLT and CFHT to detect the magnetic fields and chemical pecu- liarities in two HESs that are supposed to be the progenitors of the magnetic Ap/Bp stars. Hamaguchi et al. (2005) showed that the properties of thermal X-rays observed by the ASCA satellite are well explained by magnetic activity in the circumstellar disk of HESs.

References

LBV and central stars of planetary nebulae Chesneau, 0., Colliud, A., de Marco, 0., and 7 co-authors (2006). A close look into the carbon disk at the core of the planetary nebula CPD-56°8032. A. A., 455, 1009-1018. Chesneau, 0., Min, M., Herbst, T., and 15co-authors (2005). The sub-arcsecond dusty environment of Eta Carinae. A. A., 435, 1043-1061. Davies, B., Oudmaijer, T. D., and Vink, J. S. (2005). Asphericity and clumpiness in the winds of Luminous Bleu Variables. A. A., 439, 1107-1125. Weigelt, G., Petrov, R. G., Chesneau, 0., Davidson, K., and 21 co-authors (2006). VLTI-AMBER observations of Eta Carinae with high spatial resolution and spectral resolutions of 1500 and 10,009. Advances in Stellar Interferometry. Monnier, J. D., Scholler, M., and Danchi W. C. (eds.), Proc. The SPIE, Soc, Photo-Optical Instrumental Engineering. Bellington, WA, Vol. 6268.

Be stars Chesneau, 0., Meilland, A., Rivinius, T., and 12 co-authors (2005). First VLTI/MIDI observations of a Be star: Alpha Arae. A. A., 435, 275-287. Supplement 507

Gies, D. R., Bagnuolo, W. G., Baines, E. K., ten Brummelaar, T. A., and 21 co-authors (2007). CHARA Array K'-band measurements of the angular dimensions of Be star disks.Ap. J., 654, 527-543. Grundstrom, E. D. and Gies, D. R. (2006). Estimating Be star disk radii using H« emission equivalent widths. Ap. J., 651, L53-L56. Kervella, P. and Domiciano de Souza, A. (2006). The polar wind of the fast rotating Be star Scherner. VINCI/VLTI interferometric observations of an elongated polar envelope. A. A., 453, 1059-1066. Meilland, A. and Stee, Ph. (2006). Recent results from the SIMECA code and VLTI observations. EAS Pub. Ser., 18, 273-290. Meilland, A., Stee, Ph., Zorec, J., and Kanaan, S. (2006). Be stars: one ring to rule them all? A. A., 455, 953-961. Rivinius, T. (2005). Links between hot stars and their disks. The Nature and Evolution of Disks around Hot Stars. Ignace R. and Gayley K. G. (eds.), ASP Conf. Sere Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 178-189. Stee, Ph., Meilland, A., Berger, D., and Gies, D. (2005). Interferometic study of hot star disks. The Nature and Evolution of Disks around Hot Stars. ASP Conf. Sere Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 211-222. Tycner, Ch., Lester, J. B., Hajian, A. R., Armstrong, J. T., and 5 co-authors (2005). Properties of the Halpha-emittiong circumstellar regions of Be stars. Ap. J.. , 624, 359-371. Tycner, Ch., Gilbreath, G. C., Zavala, R. T., Armstrong, J. T., and 5 co-authors (2006). Constraining disk parameters of Be stars using Norrowband Halpha Interferometry with the Navy Prototype Optical Interferometer. A. J., 131, 2710-2721.

Mira variables Boboltz, D. A. and Wittkowski, M. (2005). Joint VLBA/VLTI observations of the Mira variable S Orionis. Ap. J., 618, 953-961. Cotton, W. D., Mennesson, B., Diamond, P. J., Perrin, G., and 10 co-authors (2005). IR and SiD maser observation of Miras. Future Direction in High Resolution As- tronomy. Romney J. D. and Reid M. J. (eds.), ASP Conf. Sere Vol. 340, Ast. Soc. Pacific, San Francisco, CA, 380. Ireland, M. J. and Scholz, M. (2006). Observable effects of dust formation in dynamic atmospheres of M-type Mira variables. M. N. R. A. S., 367, 1585-1593. Ireland, M. J., Tuthill, P. G., Davis, J., and Tango, W. (2005). Dust scattering in the Miras resolved by Optical interferometric polarimetry. M. N. R. A. S., 361, 337-344. Millan-Gabet, R., Pedretti, E., Monnier, J. D., Scholerb, F. P., and 4 co-authors (2005). Diameters of Mira stars measured simultaneously in the J, H, K' near-infrared bands. Ap. J., 620, 961-969. Ohnaka, K., Scholz, M., and Wood, P. R. (2006). Comparison of dynamical model atmospheres of Mira variables with mid-infrared interferometric and spectroscopic observations. A. A., 446, 1119-1127. Ohnaka, K., Bergeat, J., Driebe, T., Graser, D., Hofmann, H.-H., and 14 co-authors (2005). Mid-infrared interferometry of the Mira variable RR Sco with the VLTI MIDI instumemt. A. A., 429, 1057-1067. 508 Astrology of Emission-Line Stars

Wittkowski, M. and Boboltz, D. A. (2005). Joint VLTI/VLBA observations of Mira stars. Future Directions in High Resolution Astronomy. Romney J. D. and Reid M. J. (eds.), ASP Conf. Ser. Vol. 340, Ast. Soc. Pacific, San Francisco, CA, 389- 393.

Herbig Ae/Be stars Benisty, M., Malbet, F., de Wit, W. J., Kraus, S., Meilland, A., and 12 co-authors (2005). MWC 297: disk and wind spatially resolved with VLTI/AMBER. Protostars and Planets V. Proceedings of the Conf. held Oct. 24-28, in Hilton Wailoloa Village, Hawaii, LPI Contr. No. 1286. Cabrit, S., Pety, J., Pesenti, N., and Dougados, C. (2006). Tidal stripping and disk kinametics in the RW Aurigae system. A. A., 452, 897-906. Fujiwara, H., Honda, M., Kataza, H., Yamashita, T., Onaka, T., and 6 co-authors (2006). The asymmetric thermal emission of the protoplanetary disk surrounding HD 142527seen by SUBARU/COMICS. Ap. J., 644, L433-L136. Fukagawa, M., Tamura, M., Itoh, Y., Kudo, T., Imaeda, Y., and 3 co-authors (2006). Near-infrared images of protoplanetary disk arounding HD 142527. Ap. J., 636, L153-L156. Grady, C. A., Woodgate, B., Heap, S. R., Bowers, C., and 3 co-authors (2005). Resolv- ing the inner cavity of the HD 100546 disk: A candidate young planetary system? Ap. J., 620, 470-480. Honda, M., Kataza, H., Okamoto, Y. K., Yamashita, T., and 7 co-authors, SUBARU/ COMICS 24.5 micron imaging of neaby Herbig Ac/Be disks. Protostars and Planets v. Proceedings of the Conf. held Oct. 24-28, in Hilton Wailoloa Village, Hawaii, LPI Contr. No. 1286. Lin, S. Y., Ohashi, N., Lim, J., Ho, P., Fukagawa, M., and Tamura, M. (2006). Possible molecular spiral arms in the protoplanetary disk of AB Aurigae. Ap. J., 645, 1297- 1304. Millan-Gaber, R., Monnier, J. D., Berger, J. P., Traub, W. A., and 12 co-authors (2006). Bright localized near-infrared emission at 1-4 AU in the AB Aurigae disk revealed by IOTA Closure Phases. Ap. J., 645, L77-L80. Monnier, J. D., Berger, J. P., Millan-Gabet, R., Traub, W. A., and 12 co-authors (2006). Few skewed disks found in first closure-phase survey of Herbig Ae/Be stars. Ap. J., 647, 444-463. Monnier, J. D., Millan-Gabet, R., Billmeier, R., Akeson, R. L., and 30 co-authors (2005). The near-infrared size-luminosity relations for Herbig Ae/Be disks. Ap. J., 624, 832-840. Okamoto, Y. K., Kataza, H., Honda, M., Yamashita, T., and 6 co-authors (2006). Extended mid-infrared dust emission survey toward Herbig Ae/Be stars. Protostars and Planets V. Proceedings of the Conf. held Oct. 24-28, in Hilton Wailoloa Village, Hawaii, LPI Contr. No. 1286. Preibisch, Th., Kraus, S., Driebe, Th., van Boekel, R., and Weigelt, G. (2006). A compact dusty disk around the Herbig As star HR 5999 resolved with VLTI/MIDI. A. A., 458, 235-243. Raman, A., Lisanti, M., Wilner, D. J., Oi, C., and Hogerheijde, M. (2006). A Keplelrian disk around the Herbig Ae star HD 169142. A. J., 131, 2290-2293. Supplement 509

Tamura, M. and Fukagawa, M. (2005). Circumstellar disks in PMS and T Tauri stars- Herbig Ae/Be stars, Vega-like stars, and submillimeter polarizations. Astronomical Polarimetry: Current Status and Future Directions. Adamson, A., Aspin, C., Davis, C. J., and Fujiyoshi, T. (eds.), ASP Conf. Sere Vol. 343, Ast. Soc. Pacific, San Francisco, CA, 215.

T Tau stars Akeson, R. L., Walker, C. H., Wood, K., Eisner, J. A., and 6 co-authors (2005). Keck interferometer observations of classical and weak-line T Tauri stars. Ap. J., 635, 1173-1181. Duchene, G., Ghez, A. M., McCabe, C., and Ceccarelli, C. (2005). The circumstellar environment of T Tauri S at high spatial and spectral resolution. Ap. J., 628, 832- 846. Mayama, S., Tamura, M., Hayashi, M., Itoh, Y., Fukagawa, M., and 16 co-authors (2006). Subaru near infrared coronagraphic images of T Tauri. P. A. S. Japan, 58, 375-382. Millan-Gabet, R., Monnier, J. D., Akeson, R. L., Hartmann, L. and 30 co-authors (2006). Keck interferometer observations of FU Orionis objects. Ap. J., 641, 547- 555. Quanz, S. P., Henning, Th., Bouwman, J., Ratzka, Th., and Leinert, Ch. (2006). FU Orionis: The MIDI VLTI perspective. Ap. J., 648, 472-483.

Magnetic fields of early-type stars

Be stars Brown, J. C. and Cassinelli,J. P. (2005). Effects of magnetic fields on winds and disks. The Nature and Evolution of Disks around Hot Stars. Ignace R. and Gayley K. G. (eds.), ASP Conf. Sere Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 88-99. Cassinelli, J. P. and Neiner, C. (2005). Magnetic fields and Be stars. The Nature and Evolution of Disks around Hot Stars. ASP Conf. Sere Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 43-55. Maheswaran, M. (2005). A magnetic rotator wind disk model for Be stars. The Nature and Evolution of Disks around Hot Stars. ASP Conf. Sere Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 259-263. Neiner, C. and Hubert, A. M. (2005). Magnetic fields in Be stars. The Nature and Evolution of Disks around Hot Stars. ASP Conf. Ser. Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 275-278. Smith, M. A. and Balona, L. (2006). The remarkable Be star HD 110432 (BZ Crucis). Ap. J., 640, 491-504. Smith, M. A., Henry, G. W., and Vishniac, E. (2006). Rotational and cyclical variability in gamma Cassiopeia. Ap. J., 647, 1375-1386. Ud-Doula, A., Townsend, R., and Owocki, S. (2005). Centrifugal breakout of magneti- cally confined line-driven stellar winds. The Nature and Evolution of Disks around Hot Stars. ASP Conf. Sere Vol. 337, Ast. Soc. Pacific, San Francisco, CA, 319-323. 510 Astrology of Emission-Line Stars

HES Catala, C., Alecian, E., Donati, J. F., Wade, G. A., and 6 co-authors (2007). The magnetic field of the pre-main sequence Herbig Ae star HD 190073. A. A., 462, 293-301. Drouin, D., Wadem G. A., Landstreet, J. D., Mason, E., and 6 co-authors (2005). Seeking the progenitors of magnetic Ap stars: A search for magnetic fields in HAeBe stars using FORS 1 and ESPaDOnS. EAS Publ., Sere 17, 309-312. Hamaguchi, K., Yamauchi, S., and Koyama, K. (2005). X-ray study of Herbig Ac/Be stars. Ap. J., 618, 360-384. Hubrig, S., Szeifert, T., North, P., Scholler, M., and Yudin, R. V. (2005). Magnetic fields of B and Herbig Ae stars measured with FORS 1 at VLT. The Nature and Evolution of Disks around Hot Stars. Ignace R. and Galey K. G. (eds.), ASP Conf. Sere V. 337, Ast. Soc. Pacific, San Francisco, CA, 236-239. Hubrig, S., Yudin, R. V., Scholler, M., and Pogodin, M. A. (2006). Accurate magnetic field measurement of Vega-like stars and Herbig Ae/Be stars. A. A., 446,1089-1094. Yudin, R. V., Pogodin, M. A., Hubrig, S., and Scholler, M. (2006). Magnetic fields in Herbig Ae/Be stars. Convection in Astrophysics. IAU Symp. 239, held on 21-25. August, 2006 in Prague, Czech Republic, S239, 51. Yudin, R. V. (2005). Circumstellar discs around Ae/Be and Vega-type stars and local magnetic fields. The Nature and Evolution of Disks around Hot Stars. Ignace R. and Galey K. G. (eds.), ASP Conf. Sere V. 337, Ast. Soc. Pacific, San Francisco, CA, 342-345. Author Index

Letter T or F after the page number indicates the author found in the table or figure of the page.

A Bastien, P. 429, 455, 455T, 456F Abbott, D. C. 90, 91, 91F, 195 Batalha, C. C. 465, 466F Aiad, A. 476, 477f Bath, G. T. 386 Albright, G. E. 354, 354F Batten, A. H. 229 Alencar, S. H. P. 488 Bauer, W. H. 359F, 360 Allen, D. A. 251, 274, 275T, 398T, 398, Baum, E. 197 399 Beals, C. S. 11, 198, 281, 282F Aller, L. H. 36, 61, 69, 141, 220T Behr, A. 246 Ambartsumian, V. A. 329, 337, 448 Belcher, J. W. 96 Anandarao, B. G. 399 Belczynski, K. 398 Anderson, Ch. M. 399, 400F Bell, K. R. 475F Anderson, L. S. 179 Bellingham, J. G. 470 Andrillat, Y. 219, 219T, 227, 255, 256, Benedettini, M. 484, 486, 486F 256F Bennett, P. D. 360 Anupama, G. C. 382, 383F, 384T, 393 Beristain, G. 490, 491F Apparao, K. M. V. 258 Bertout, C. 471,476 Appenzeller, I. 453, 460,.462, 462F, 488 Bertschinger, E. 99 Arkhipova, V. P. 405, 406F Beskrovnaya, N. G. 431, 442 Armitage, P. J. 114, 115F, 494 Bhatt, H. C. 431 Ashok, N. M. 254, 255, 255F Bibo, E.A. 438, 439F Athey, R. G. 179 Bidelman, W. P. 224 Attridge, J. M. 467, 467T Bjorkman, K. S. 248, 249F Audard, M. 329 Bleau, W. J. 282 Bloch, M. 373, 373F, 380 B Bode, M. F. 382, 384T, 404 Baade, D. 270 Bohannan, B. 276, 276F Baker, J. G. 138, 140 Bohm, T. 183, 424, 427, 435, 436F, 442, Bakos, A. G. 262 442F, 444, 445 Ballereau, D. 266 Bohm-Vitense, E. A. 343 Balona, L. A. 273, 274 Bohn, H. U. 130T Bappu, M. K. V. 7, 321, 322F, 340F, Bond, H. E. 222 341T Bopp, B. 325 Baratta, G. B. 406 Bord, D. B. 350 Barbier, D. 25 Bouret, J. C. 427, 445 Barker, P. K. 240, 241F Bourvier, J. 463, 465F, 467, 471 Basri, G. 465, 466F, 488 Bowen, I. S. 11, 171

511 512 Author Index

Bowen, G. H. 350 Corcoran, M. F. 197, 211 Brandt, J. C. 96 Corporon, P. 437, 437T Breger, M. 429 Cote, J. 251 Briot, D. 229, 234, 235F, 296 Cox, A. N. 29T Brocklehurst, M. 142 Coyne, G. V. 246 Brown, A. 465 Cram, L. E. 179, 180, 181, 181F, 325, 465 Bruevich, E. A. 146, 335, 337F Crawford, D. L. 20T Budding, E. 352, 355F Crowe, R. A. 343, 344T Bunsen, R. 9 Crowther, P. A. 213, 214T Burgers, J. M. 13 Cuntz, M. 130, 179 Burwell, C. G. 226, 397 Byrne, P. B. 366 D Dachs, J. 234, 235, 235F C Damiani, F. 7.1.5 Cabrit, S. 453, 471, 472 D'Antona, F. 412 Cakirli, 6 365 Davidson, K. 275, 278, 287 Calvet, N. 466F Davis, L. Jr. 92, 95, 96F Campbell, W. W. 4 de Groot, M. 278, 284 Cannon, A. J. 5, 6, 6T, 8 de Jager, C. 293, 329, 330F Canto, J. 447 De Marco, 0.222 Carlberg, R. G. 127 Deslandres, H. A. 7 Cassinelli, J. P. 75, 89, 92, 260, 261F, 295 Deutsch, A. J. 14 Castelaz, M. W. 350 de Winter, D. 274 Caster, J. I. 75, 90, 161, 162, 162F, 212 de Zeeuw, P. T. 192 Catala, C. 183, 424, 427, 435, 436F, 442, Divan, L. 25, 26, 27F 443, 443F, 444, 445, 446 Doazan, V. 226, 266 Cerruti-Sola, M. 223, 224F Dobrzycka, D. 380, 396 Chalonge, D. 25, 26, 27F, 373, 373F Dominik, C. 98 Chambers, H. L. 348 Dougherty, S. M. 195, 204 Chandrasekhar, S. 74 Downes, R. A. 393, 394F, 395, 397 Chaubey, U. S. 296 Doyle, J. G. 325, 328 Chauville, J. 65, 232, 266 Drake, S.A. 144, 144F, 145, 146F, 235, Cheng, Q. Q. 176, 177, 179, 321 236, 396 Cherepashchuk, A. M. 208, 210 Dufay, J. 380, 381F Chevalier, R. A. 99 Chin, C. W. 295 E Chincarini, G. 374, 374T Eberhard, G. 7 Choi, H. J. 320, 320F Echevarria, J. 396 Ciardullo, R. 222 Elitzur, M. 142, 397 Cidale, L. 275 Emerson, D. 155 Cohen, D. H. 240, 260, 261F Emerson, J. P. 460, 461F Cohen, M. 213, 215T, 449, 449T, 450, Endal, A. S., 343 455, 456F, 457, 458F, 479, 479T, 480, Engvold, O. 321 481F Ergma, E. 210 Collins, H.G. W. 232, 234, 235F Etzel, P. B. 355, 355F Conti, P. S. 106, 106F, 190, 191, 192T, 193F, 202, 215, 215T, 216, 216T, F 217F, 219, 219T, 275 Fabregat, J. 297 Contini, M. 383, 402 Feibelman, W. A. 222 Author Index 513

Feinstein, A. 262, 296 Hamann, W. R. 169, 170, 190, 212, 213, Fekel Jr., F. 325 214T Feldmeier, A. 128, 128F Hanuschuk, R. W. 226, 268, 269F Felli, M. 196, 196F, 197, 197T Harmanec, P. 229, 259, 273, 300 Fernandez, M. 477, 478F Haro, G. 329, 337, 338 Finkenzeller, U. 424, 425T, 426F, 435, Harrop-Allin, M. K. 114 444, 487 Hartigan, P. 472, 472F Fleming, W. 5, 5T, 6 Hartmann, L. 101, 111, 112F, 113F, 319, Folha, D. F. M. 460, 461F 324, 325, 325T, 326F, 339, 339F, Formiggini, L. 410 476T, 493, 494F Fox, M. W. 344T, 344F, 346, 346T, Hessman, F. V. 389, 390F 348F, 349F Hearn, A. G. 92 Fraunhofer, J. von 3 Helfand, D. J. 350 Frew, D. J. 278 Henyey, L. G. 12 Frost, S. A. 216, 217F, 219 Herbig, G. H. 7, 8, 318, 423, 449, 449T, Fukuda. 1. 66, 66F, 219T, 231, 435, 452, 454, 469, 474, 476 436F Herbst, W. 319, 319F, 440, 450, 467, 467T, 469F, 470 G Hernandez, J. 424 Gabler, A. 75 Herzberg, G. 36 Gahm, G. F. 453, 453T, 470, 471 Hertzsprung, E. 8 Gail, H. P. 97, 98 Hill, S. J. 99, 100F Gallagher III, J. S. 291, 291F, 292 Hillier, D. J. 212, 280 Garcia-Alvarez, D. 336 Hillenbrand, L. A. 425T, 427, 428T Garmany, C. D. 106, 106F Hirata, R. 229, 232F, 239, 248, 265, Garrison, R. T. 343, 344T 265F, 266 Gauzit, J. 408 Hirth, G. A. 473, 474F Gehrz, R. D. 251 Hoffiich, P. 487F Gershberg, R. E. 329, 334, 335, 335T, Hoffmeister, C. 343, 366, 366F, 367F, 394, 395T, 401, 484 379T . Ghandour, L. 445 Holzer, T. E. 102, 102F Ghez, A. M. 468 Honeycutt, R. K. 353 Ghosh, K. K. 248 Horaguchi, T. 259, 266, 267F Giampapa, M. S. 179, 180, 181F, 182 Horne, K. 170, 384F, 385, 386, 388 Gill, C. D. 375, 377F, 378F 388F Gillet, D. 125, 126F, 347, 349T Houdebine, E. R. 325, 327F, 332 Gilroy, K. K. 218 Howarth, 1. D. 202 Giovanardi, C. 484, 485F, 486, 487F Huang, S. S. 65, 239, 268 Glasby, J. S. 440 Hubble, E. 290 Gliese, W. 328, 328T Hubeny, J. 249 Gomez, A. E. 20 Hubert, H. 226 Gray, D. 66,343 Hubert-Delplace, A. M. 226, 262 Grinin, V. P. 430, 430F, 438, 482, 483 Huggins, W. 3, 4, 11 Gutierrez-Moreno, A. 155,401 Hugoniot, H. 12 Humason, M. L. 8 H Hummel, W. 239 Hack, M. 356, 357T, 360 Hummer, D. G. 75, 143, 163 Hagen, W. 360 Humphreys, R. M. 275, 276F, 278, 287 Hamann, F. 429 Husfeld, D. 169 514 Author Index

I Kolotilov, E. A. 440, 441F, 479, 479T, Iben, Jr., I. 115, 412 482 Ichimura, K. 331 Konigl, A. 111 Ignace, R. 198 Kopal, Z. 351 Iijima, T. 380, 382 Koppen, J. 480, 480T, 483, 483T Ikeda, Y. 407, 408F, 409F Kosirev, N. A. 74 Illarionov, A. F. 404 Kraft, R. P. 375 Imhoff, C. L. 460, 462, 462F Kriz, S. 229, 268 Inglis, D. R. 61 Kron, G. E. 20T Ivison, R. J. 403 Kruszewski, A. 246 Kudritzki, R. P. 73 J Kuhi, L. V. 198, 200F, 449, 450, 450F, Jain, S. K. 431 455, 456F, 457, 458F, 479, 479T, 480, Jankovics, I. 487 481F Jaschek, M. 224, 229, 239 Kukarkin, B. V. 344T, 352, 398T, 440 Jaschek, C. 229, 239 Kunasz, P. B. 168 Jeffery, D. 163 Kunjaya, Ch. 248 Johns-Krull, C. M. 462, 463F Kunkel, W. E. 331, 331F, 332T, 335 Johnson, H. L. 19, 20T Kurucz, R. L. 71, 72, 72F, 73F, 251, Jorissen, A. 116, 116F 252F Joy, A. H. 7, 8, 9T, 350, 448 Kwok, S. 97 Jura, M. 350 L K la Dous, C. 393 Kahn, F.D. 382, 384T Lafun, J. ~ J. 125, 126F Kaitchuck, R. H. 353 Lamers, H. J. G. L. M. 89, 92, 162, 163, Kambe, E. 270, 271F 212, 218, 218T, 274, 277,278T, 283F, Karovska, M. 350 284, 285F, 286F Kato, S. 268 Landsman, W. B. 182, 183F Katsova, M. M. 336 Landstreet, J. D.·430, 455 Katysheva, N. A. 480 Lang, K. R. 23T Kawabata, S. 357, 358F Langer, N. 293 Keenan, P. C. 23T, 24, 343 Lauterborn, D. 352 Kenyon, S. J. 291, 291F, 292, 397, 405T, Lawson, W. A. 274 406, 409, 410T, 476T Leep, E. M. 215, 215T, 216T, 219, 219F Kharchenko, N. 343 Leedjarv, L. 404 Kingsburg, R. L. 190, 191T Leinert, Ch. 468 Kippenhahn, R. 85, 86F, 352 Leitherer, C. 105, 106, 106e, 218, 218T, Kirchhoff, G. 3, 9, 10 277 Kirkpatrick, J. D. 24 Lepine, S. 208 Knapp, G. R. 107, 108, 344T Leung, K. C. 353 Kneer, F. 314 Leynolds, O. 13 Koesterke, L. 213, 214T Li, W. 435 Kogure, T. 149, 150, 153, 163, 229, Lim, J. 107 230F, 232F, 236, 237, 237F, 238F, Liu, Q. Z. 258 239, 242F, 244F, 262, 263F, 264, Livio, M. 114, 115F, 379T 264F Lopez, J. A. 412 Kohler, R. 468 Loup, C. 108 Kohoutek, L. 221T Lucy, L. 90 Author Index 515

Lundstrom, I. 198, 199F Moffat, A. F. J. 205, 207, 207F, 208, 209, Luttermoser, D. G. 350 210 Montes, D. 361, 361T, 362, 363F M Morales-Rueda, L. 385 MacGregor, K. B. 96, 101 Morgan, W. A. 24, 25, 337 Mach, E. 12 Moreno, H. 155, 401 Maeda, Y. 211 Morris, M. 107, 108 Maeder, A. 208, 209F, 278, 293,.295, Morris, P. W. 194 411 Morse, J. A. 279, 279F Maehara, H. 350, 404 Mullan, D. J. 107, 176, 177F, 179 Magazzu, A. 454, 454F Munari, U. 398, 399T Maheswaran, M. 295 Mundt, R. 423, 424, 425T, 426F, 444, Malfait, K. 424, 429 447, 447T Marchenko, S. V. 210, 212F Muratorio, G. 289 Markova, N. 281, 282, 283F, 284 Muzerolle, J. 446, 489, 489F, 490F Marlborough, J. M. 163, 248, 249, 255 Marsh, T. R. 170, 385 N Martin, E. L. 435, 454 Negueruela, I. 219, 219T, 259 Martinez-Pais, I. G. 386, 387F Neuhauser, R. 462, 463, 463T, 464, 464F Mason, E. 396 Newman, M. J. 108, 109F Mathieu, R. D. 468 Niedzielski, A. 201, 201F Matthews, H. E. 447 Nieuwenhuijzen, H. 123, 124, 125F, 293 Mauas, P. J. D. 176 Nisini, B. 484, 485, 486, 487F Maunder, E. W. 5 Nussbaumer, H. 410, 411, 411e Maury, A. C. 5,22 Mazzitelli, I. 412 o McDavid, D. 248 O'Brien, T. J. 375, 377F, 378F McLaughlin, D. B. 369, 371F Okazaki, A. 268 Meier, S. R. 398T, 402, 403F Oliverson, N. A. 399, 400F Melo, C. H. F. 468 Olson, E. C. 115, 355, 355F Menard, F. 455, 457F Osaki, Y. 270, 273, 386 Mendez, R. H. 222, 223F Osten, R. A. 331 Mendoza, C. 174T Ostriker, E. C. 111 Mendoza, E. E. 262, 457 Owocki, S. P. 208, 213 Mennickent, R. E. 233, 234F, 239 Ozeren, F. F. 321 Menzel, D. H. 10, 11, 138, 140 Merrill, P. W. 6, 7, 14, 32, 226, 228, 397, p 408 Paczynski, B. 113 Meyer, M. R. 460 Palla, F. 492, 492F, 493, 493F Meynet, G. 293, 295 Pallavicini, R. 450 Mihalas, D. 73, 74F, 75, 166,168 Panagia, N. 196, 196F, 197, 197T Mikolajewska, J. 393 Papkalla, R. 168 Mikolajewski, M. 404 Parenago, P. 344T, 352, 398T, 440, 469· Miller, D. L. 212 Parker, E. N. 13 Miller, J. R. 319, 319F Parsamian, E. S. 329, 334, 334F Miroshnichenko, A. S. 259 Payne-Gaposchkin, C. 369 Mirzoyan, L. V. 338, 338F Pena, M. 222 Mitchell, G. F. 447 Penny, L. 216, 217T, 219 Miyamoto, S. 12, 13, 147, 150, 236 Percy, J. R. 262, 270 516 Author Index

Perek, L. 221T Rochowicz, K. 201, 201F Perez, M. R. 427, 445, 446 Rodono, M. 332, 333F Perinotto, M. 223, 224F Romanishin, W. 296 Persson, S. E. 429 Rons, N. 166 Peters. G. J. 249, 353 Roques, P. 8 Petit, M. 368T Rosino, L. 374, 374T, 382 Pettersen, B. R. 323 Rossano, G. S. 470 Pickering, E. C. 5, 5T, 22 Rosseland, S. 11, 12, 136 Pikel'ner, S. B. 14 Rountree, J. 249 Pirzkal, N. 436, 437, 437T Rybicki, G. B. 163, 169 Planck, M. 10 Rydgren, A. E. 458, 459F Plavec, M. 229, 353, 353T Rygh, B.O. 319 Poe, C. H. 208, 213 Poeckert, R. 248, 255 S Polidan., R. S. 229, 353, 353T Saijo, K. 359 Pollock, A. M. T. 197 Saito, M. 359 Pols, O. R. 300, 300T, 301 Sandage, A. 290 Pontefract, M. 430 Schaller, G. 293, 294F Portegies Zwart, S. F. 301 Schatzman, E. 14 Porter, J. M. 225 Schild, H. 405, 406 Pottasch, S. R. 141, 141T, 142, 142T, Schild, R. 296 152, 152F, 220, 220T, 221, 221T, Schmid, H. 405, 406 236 Schmitz, F. 179 Prabhu, T. P. 382, 383F, 384T Schmutz, W. 170, 202 Praderie, F.' 444 Schrijver, C. 176, 177F Preibisch, Th. 425T, 431, 434F, 445 Schulte-Ladbeck, R. A. 198 Preston, G. W. 317, 318F Schwank, ~. 401, 401F, 402F Proudman, I. 82, 84 Schwarzschild, K. 9 Seaquist. E. R. 403 Q Secchi, A. 3, 4 Quirrenbach, A. 246 Sedlmayer, E. 97, 98 Seggewiss, W. 202 R Seitter, W. C. 369 Rankine, W. J. M. 12 Shafter, A. W. 389, 390F, 391, 392F Rao, N. K. 449 Shara, M. M. 205, 378 Rappaport,S. 258 Shawl, S. J. 350 Ratering, C. 389 Shnol, E. E. 335, 394, 395T, 401, 484 Rauw, O. 208, 209F Shore, S. N. 382, 383 Ray, T. P. 447, 447T, 448F Short, C. I. 328, 366 Rayet, G. 4, 189 Shu, F. H. 111 Reid, I. N. 24 Simon, T. 182, 183F Reipurth, B. 468, 488 Singh, M. 296 Richards, M. T. 115, 354,·354F Skinner, S. L. 205,433, 434, 435F, Rinehart, S. A. 257, 257T 445 Ritter, H. 368T Slavin, A. J. 375 Rivinius, Th. 225, 243, 245 Slettebak, A. 228, 228T, 229, 233, 234, Robert, C. 205 234F, 235, 235F, 249 250F, 296, Robinson, E. L. 366 297F Robinson, R. D. 259 Smith, L. F. 198, 200F, 208, 209F Author Index 517

Smith, L.J. 278T Townsend, R. H. D. 233 Smith, M. A. 250, 259, 273 Truran, J. W. 379T, 406 Snow, T. P. Jr. 92, 253F Turner, C. G. 66 Sobolev, V. V. 12, 155, 160, 161 Tutukov, A. V. 412 Soker, N. 278 Tycner, Ch. 245, 245T Solomon, P. H. 90 Tylenda, R. 221 Sonneborn, G. 249 Sorelli, C. 446 U Stahl, O. 284, 289, 289T Uesugi, A. 219T, 435, 436F Stahler, S. W. 108, 110F, 492, 492F, Ulmschneider, P. 83, 84, 84F, 85F, 130, 493F 131F, 179 Starrfield, S. 377 Ulrich, R. K. 144, 144F, 145, 146F, 235, Stauffer, J. R. 318, 324, 325, 325T, 326F, 236,282,396 339, 339F Underhill, A. B. 208, 210, 211T, 213, Stebbins, J. 20 216, 218 Stein, R. F. 83 Unsold, A. 63, 65F Stella, L. 258, 258T Stelzer, R. 463 V Stencel, E. R. 360 Vacca, W. D. 191, 192T, 193 Stenholm, B. 19~, 199F Van Altena, S. F. 20 Stepien, K. 130 van Bever, J. 301 Stibs, D. W. N. 169 Vanbeveren, D. 361 Stickland, D. J. 391, 392F van Blerkom, D. 161, 162F, 212 Stothers, R. B. 295 van den Ancker, M. E. 274 Strassmeier, K. G. 341, 342F, 361, van den Heuvel, E. P. J. 258, 298F, 299, 361T 299T Stripe, G. M. 145 van der Hucht, K. A. 190, 191T, 192, Strom, S. E. 423 192T, 194, 194F, 202, 203F, 204F, Stromgren, B. 20 205, 205T, 209, 221T Struve, O. 11, 13, 65, 226, 227F, 268 Van de Hulst, H.C, 13 Sunyaev, R. A. 404 van Genderen, A. M. 205, 206, 206F, Swings, J.P. 274, 275T 208, 280 Szeifert, Th. 291, 292, 292T van Kerkwijk, M. H. 210, 255 Van Maanen, A. 8 T Vaughan, A. H. 317, 318F Takeda, Y. 66 Vink, J. S, 429, 430, 433F, 457 Tamura, S. 407, 408F, 409F Viotti, R. 278, 279, 280e, 405T, 406 Tappert, C. 389 Vladilo, G. 319 Tarasov, A. E. 231 Vrancken, M. 239 Taylor, A. R. 240 Vrba, F. 429 Teller, E. 61 Vreux, J. M. 202, 208, 210, 213 Telting, J. 272, 272F The, P. S. 424, 425T, 427, 435, 438, W 439F, 440F,445 Walborn, N. R. 215, 215T, 216T, Theuns, T. 115, 116F 278T Thorn, C. 245 Walker, M. F. 270, 375,476 Tjin A Djie, H. R. E. 488 Wallerstein, G. 14, 280 Torrej6n, J. M. 297 Walter, F. M. 450, 452F, 480, Torres-Dodgen, A. V. 193 482F 518 Author Index

Warner, B. 114, 169, 366, 379T, 385, Wood, K. 247, 247F, 248 386T, 389, 391T Wood, P. R. 99, 346, ,348F, 349F Waters, L. B. F. M. 251,252, 252F, Woolley, R. v. d. R. 169 253F, 255, 285, 487, 487F Webbink, R. F. 379, 379T y Weber, E. J. 92, 95, 96F Yamashita, Y. 40, 350, 404 Wehrse, R. 487F Young, A. 323, 324F, 328, 328T Weigert, A. 352 Yudin, R. V. 225, 232, 233T Werner, K. 169 Yungelson, L. R. 210 Wesselius, P. P. 285 Weymann, R. 97 Z White, N. E. 259 Zak, D. S. 458, 459F White, R. C. 195 Zamanov, R. 281 White, S. M. 107 Zanstra, H. 10 Williams, P. M. 194, 194F, 195, 202, Zhai, D. S. 362, 364, 364F, 365F 204F, 205 Zhang, X. B. 362, 364, 364F, Williams, R. E. 370, 372, 372F, 374, 375, 365F 376F, 382, 396, 396T Zhekov, S. A. 205 Willson, L. A. 99, 100, 100F, 453 Zickgraf, F. J. 274, 287, 287T, 288F, 289, Wilson, O. C. 7,321, 322F, 340F, 289T, 290, 295 341T Zinn, R. J. 74F Winkler, K. A. 108, 109F Zinnecker, H. 425T, 431, 434F, 444, 445, Wolf, B. 284, 291, 292 468 Wolf, C. 4, 189 Zorec, J. 229, 290, 296 Wood, B. E. 350 Zwitter, T. 398 Subject Index

The letter T or F after the page number denotes the subject found in Table or Figure of the page.

A ATLAS1272 Absolute magnitude 20 Atmospheric eclipse 356, 357T (Flare stars) 338F (WR stars) 193, 193F B (LBV) 275 Balmer decrement 12, 140, 154 (DNe) 384F, 385 (Static envelope) 145, 146F Accretion disk/flow 108, 113 (Movingenvelope) 335, 394, 395T, 484 Spherically symmetric accretion 108, (LTE model) 335 109F (Nebular approximation) 140, 141T, Magnetospheric accretion 112, 489 142T, 396, 397, 482 Accretion disk/flow in stars (Envelope approximation) 483, 483T (Binary system) 113, 115F, 116F (Accretion disk) 396, 396T (Mira) 350 Balmer decrement in stars (CVs) 366, 372, 377, 380 (Emission-line stars) 153 (Symbiotic) 404, 405F, 409 (Be stars) 150, 152F, 233, 235F, 237F (Protostars) 110 (B[e]) 289 (HES) 434, 445, 446 (dMe stars) 334, 336 (TTS) 112, 113F, 429, 460, 471 (Flare stars) 331, 332T, 334, 335T Acoustic spectrum/power 83, 84F (Mira variable) 346, 348T, 349T Activity index 317, 318F (RS CVn) 366 Ae star 224, 226, 229 (Cataclysmic variables) 393, 394, 394F AGB (asymptotic giant branch) 108, (Symbiotic stars) 399, 401, 402F 404, 412 (HES) 479, 479T, 480T Alfven waves 101, 101F (TTS) 480, 481F Algol eclipsing binary 114, 115, 352 Balmer jump/discontinuity 25, 25F, 476 Algol star/system 229, 231, 354, 355F Basal atmosphere 175, 179, 321 Approximate lamda iteration (ALI) BCD classification -+ Spectral method 168, 212 classification Association Be star 12 OB association 190, 192T (Classical) Be stars 224, 228T, 423, T association 449 424, 444 Chamaeleon association 468 Ordinary Be stars 226, 239 Orion association 334, 337, 337F, 370 Peculiar Be stars 274, 275T Association NGC 2264 338, 338F B[e] stars 287, 287T, 289T, 295 ATA (Australia Telescope Array) 433 Be/X-ray binary 258, 258T, 300

519 520 Subject Index

Be star (cant.) GCVS (General catalogue of variable Be-shell stars 226, 240, 244F, 262, stars) 344T, 352, 398T, 440 263F HD (Henry Draper catalogue) 6 Binary. stars HDE (Extended HD catalogue) 24 WR binaries 208, 210, 299 HRC (Herbig-Roo catalogue) 449T Algol binary/system 114, 300, 352, MWC (Mount Wilson catalogue) 226, 355F, 440, 469 398 Close binary 113, 351F, 366 New Yale Catalogue (Trigonometric Eclipsing binary 114, 351, 437, 437T parallax) 20 Be/X-ray binary 258, 258T, 300, 300T Catalogue of stars for stellar type Binary of atmospheric eclipse 356, (WR) 190, 192 357T (Be) 226 Binary system/binarity in stars (UV Cet-type stars) 329 (WR) 190, 192T (Mira variables) 343 (Of) 217 (Algolsystems) 352 (PNCS) 222 (RS CVn systems, CABS) 398 (Be) 228T, 229 (Symbiotic stars) 399 (dMe) 325 (HES) 424 (Flare stars) 329 (TTS) 449, 470 (Mira variables) 350 CFHT --+ Observatory (Symbiotic stars) 408, 410T Chemical abundance/chemical (HES) 435, 437T composition (TTS) 468 (WR) 212, 214T, 215T Birthline 492 (Of) 215 Black body 10, 41, 46 (LBV) 280 Blueing effect 438 (Novae) 411F, 412 Bolometric magnitude/luminosity 21 (Symbiotic novae) 410, 411F (LBV) 275 Chromoshere 13 (Be) 260, 261F Chromospheric activity 85, 107, 176, (RES) 431, 434F 18~ 317, 319, 360, 427, 446 (TTS) 463 Chromospheric emission line 7, 180, Boltzmann's law/distribution 42 180T, 323 Boundary layer 111, 112F Models of chromosphere 179, 465, Break-up velocity 231, 232F 466F Brown dwarf 24 Color index 19, 26, (Late type stars) 319 C (Flare stars) 339, 339F CABS == Chromospherically Active (Symbiotic stars) 398, 399T Binary System ---+ Catalogue Co-movingframe method (CMF CAK ---+ stellar winds (theory) method) 166 Cataclysmic variable stars (CVs) 170, Compact stars 366, 393 (WR stars) 208, 210 Catalogue (Be) 258, 300 BSC (Bright Star Catalogue) 229, 296 Complete linearization method 212 CABS (Chromospherically active Convection layer 79, 82, 85, 319, 454 binary stars) 361 Corona 13, 89, 323 Catalogue of spectroscopic binary Coronal emission line/coronal lines systems 229 372, 374, 382 Draper Memorial Catalogue 5 Coronal X-rays 323, 383 Subject Index 521

Co-rotation circumstellar material 273 Sobolev type probability = Escape Curve of growth 66, 68F, 69, 69F probability by motion 12 Sobolev-P method 163 D Evolutionary state/scenario, of Depolarization stars (Be) 246, 248 (stars) 85, 86F (HES) 430 (Massive stars) 292, 294F, 299 Dilution factor 135, 136T, 138, 146 (Be) 296, 300 Discrete absorption component (CAC) (LBV) 280 (Be stars) 250 (dMe) (age effect) 339, 339F Doppler tomography 170, 389 (Flare stars) 337 Dust shell (envelope) .(Novae) 412 (WR) 202 (Planetary nebulae) 412 (Be) 251 (Symbiotic stars) 410 (B[eD 287 (TTS) 485 (Symbiotic stars) 399 (Pre-main sequence stars) 7, 492, (HES) 430,431,438 492F, 493 (TTS) 457 (Protostars) 108, 110F EXor star 475, 494, 494F E E/C variation (Be) 262 F Eddington approximation 54, 55, 149 Flare star 8, 328, 328T Edington-Barbier relation 52,56, 57, 62 Fluorescence line 452, 453T Eddington (luminosity) limit 98 Fluorescense mechanism Einstein coefficient 38, 43, 137, 140 (Nebula) 10 Einstein Observatory ~ X-ray satellite (TTS) 452 Equilibrium Forbidden line 11, 35, 171, 172 Thermodynamic equilibrium (TE) 10, Nebular-type forbidden lines 171 41, 46, 137 Semi-forbidden line (Intersystem lines) Detailed balancing 41, 43 175, 176T, 403 Local thermodynamic equilibrium Critical electron density 172, 174T, (LTE) 10, 47, 52, 54, 71, 80 370, 427 Non local thermodynamic equilibrium Forbidden lines in stars (Non-LTE) 10, 71, 180 (WR) 202 Thermal equilibrium 52 (Be) 274, 275T Radiative equilibrium (RE) 53 (B[e] stars) 275, 287, 290 Statistical equilibrium 139, 144, 148 (LBV) 280 Escape probability 10 (P Cyg stars) 281 Escape probability by motion 12, 155, (HS variables) 291 160, 161, 394, 395T (Atmospheric eclipse) 357 (Cataclysmic variables) 394 (VV Cep) 359 (TTS) 489 (Novae) 370, 382, 396 (Pre-main sequence stars) 484 (Symbiotic stars) 399 Escape probability by scattering 142, (Symbiotic novae) 406 144F (HES) 424, 427 (Flare stars) 336 (TTS) 453, 472, 474F (Cataclysmic variables) 396 Fraunhofer lines 3, 10 Escape probability by multiple FU Ori type star (FUor) 472, 475F, scattering 335, 337F 476T, 494, 494F 522 Subject Index

G (Be) 251, 255, 256F Gray atmosphere 54, 74 (HES) 429 Grotrian diagram 31, 40 (TTS) 457, 484 CaII35F Inglis-Teller formula 61 Fe I 452F Instability HI32F Disk instability 386 HeI37F Raylergh-Taylor instability 127 NaI34F Sound-wave instability 127 Mass-tranfer instability 386 H Pulsational instability 85 Harvard classification ---+ Spectral Wind instability 197, 208 classification Interferometry/interferometer 245, Herbig-Haro objects 446,447 245T Herbig Ae/Be (HES, HABE) 8, 423, Interstellar absorption 154, 193 425T Infrared Space Observatory (ISO) ~ Hipparcos satellite/parallax 20, 192 Infrared satellite HR (Hertzsprung-Russell) diagram 1, IUE satellite/observations ---+ Ultraviolet 2F, 26, 28F, 276F, 285F satellite HII region (WR) 191, 192T J (Symbiotic stars) 401, 401F Jet flow/stream 404,446, 447T, 448F, HMXB (High mass X-ray binary) 258, 471, 473 298F, 299 Hubble-Sandage variable (HS variable) K ~ Variable stars Keplerian motion 239 Hubble Space Telescope (HST) 182, Kirchhoff-Bunsen's experiment 55 183F, 222,279, 279F, 291, 350, Kirchhoff's law 10, 47 412 Hugoniot curve ---+ Rankine-Hugoniot L relation Lagrangian point 113, 114F Humphrey-Davidon instability limit 275, Lamda operator (A-operator) 168 276F, 284, 285F Approximate A-operator (ALI method) 169 I LBV (Luminous blue variable) 275, Infrared excess 276F, 278T, 293 (WR) 195, 202 Limb darkening 49 (Be) 251, 254 Linear polarization (B[e]) 274, 287 (Be stars) 246, 247F, 249F (Mira variables) 410 (HES) 423, 429 (Symbiotic stars) 399, 410 (TTS) 455, 455T, 456F (HES) 423, 427 Lithium (Li) abundance 449, 454, (TTS) 460, 471 454F Infrared satellite Local thermodynamic equilibrium IRAS (Infrared Astronomical (LTE) ---+ Equilibrium Observatory) 251, 399, 429 LTE model/LTE state ISO (Infrared Space Observatory) 202, Stellar atmosphere 52, 71, 72F, 73F 203F, 209, 484, 486 Flare stars 335 Infrared spectrum Cataclysmic variables 396 (WR) 202, 203F Luminosity class 24, 224 Subject Index 523

M Recurrent nova (RN) 378, 379T Magnetic accretion flow Dwarf nova (DN) 385, 386T (TTS) 489 Nova-like variables (NL) 389, 391T (HES) 446 Symbiotic nova 404, 405T Magnetosphere 404, 446, 489 Mass-accretion rate o (Symbiotic stars) 409 Observatory (TTS) 463F, 474, 494, 494F Asiago Observatory 373, 382 Mass-loss rate 104 Beijin Astronomical Observatory (Early-type stars) 104, 106F (Xinglong Station) 362 (Late-type stars) 107 Calar Alto Observatory 473, 478 (Massive stars) 293, 294F Cerro Tololo Interamerican (WR) 211 Observatory (CTIO) 350 (Of) 218, 218T Canada-France-Hawaii Telescope (Be) 251, 253F, 487F (CFHT) 207 (LBV) 277, 280 Colorado University Observatory 241F (PNCS) 223, 224F Cote D'Azur Observatory 245 (P Cyg stars) 284, 286F Crimean Observatory 441, 442 (HS variables) 291, 292T ESO (European Southern (dMe) 107 Observatory) 223, 279, 287, 288F (Mira variables) 410 Harvard College Observatory 5 (VV Cep) 359 Haute Provence observatory 255, 373, (Symbiotic stars) --+ (Mira variables) 373F, 380, 381F (HES) 434, 487F Kitt Peak Observatory 471, 472 (TTS) 453, 471, 484, 486, 487F Kuiper Airborn Observatoy (KAO) (YSO = Young stellar object) 487f 428F MCAK --+ stellar winds (theory) Lick Observatory 4, 453 Method of velocity zones 163 Mauna Kea (CFHT, UKIRT) 207,460 Miln-Eddington model 10 Mt. Hopkins Observatory 291,324 Model atmosphere 70 Mt. Lemon Observatory 390F, 392F LTE-model 71, 72F, 73F Mt. Stromlo Observatory 346 Non-LTE model 72, 74, 180 Mt. Wilson Observatory 6, 11, 341 Extended atmosphere 74 National Radio Observatory at Kitt Unified model 75 Peak 447 Okayama Astrophysical Observatory N 40, 265F, 270, 331, 357, 407 Nebula ORM == Observatorio del Roque de Planetary nebula 220, 220T Los Muchachos (Canary Islands) Reflection nebula 279, 279F, 430, 447 375 Nebular approximation 138, 141 Paris Observatory 4 (Be stars) Roman College Observatory 3 (cataclysmic variables) 397 South-African Observatory 392F (Pre-main sequence stars) 482 Vainu Bappu Observatory 382 Non-radial pulsation (NRP) Washington Observatory 400 (WR) 208, 210 Whipple Observatory 424 (P Cyg) 284 Wyoming IR Observatory 436· (Be) 270, 272F, 296 Yerkes Observatory 12 Novae 1-4 Oe star 219, 219T, 224 Classical nova (CN) 367, 368T, 412 Of stars 155, 215, 215T, 285F, 293 524 Subject Index

One-arm oscillation 268 Be-star type 147, 150 Orion Spectrum 370 Radiative equilibrium 53 Radiative transfer 11, 44, 49 p Radio flare 331 P Cyg-type stars 11, 13, 284, 285F Radio emission P Cyg profile 162, 280, 281F; 282F Thermal emission 195 (LBV) 276, 280 (WR) 195 (P Cyg stars) 284 (RS CVn) 360 (PNCS) 220, 223F (HES) 433, 435F, 445 (Be) 249 Radio spectrum (B[e]) 289 (WR) 195 (Mira variable) 350 (Symbiotic stars) 403 (CVs) 369, 374, 380 Rankine-Hugoniot relation (RH relation) (HES) 424, 442, 444 120 (TTS) 460 Hugoniot curve 120, 121F, 123F Inverse P Cyg profile 282, 284, 444, Generalized R-H relation 122, 445, 460, 476 125F Phase variation/change Rayleigh-Jeans approximation 42 (Be stars) 261, 262, 263F, 264F, 266 Recombination/recombination line (Algols) 354, 354F 138 (Mira variables) 345F, 346 Red dwarf emission-line star (dMe) 7, (VV Cep) 357, 358F 323, 326F (Dwarf nova) 387, 387F Red giant 340, 341T, 401,412 (Symbiotic stars) 407, 408F Roche lobe 113, 351, 351F, 360 Photometric system 20T Roche equipotential curves 114F Planck function 41 Roche lobe overflow (RLOF) 113, 229, Planetary nebulae 3, 220, 220T, 221T, 300 350, 412 Rosseland cycle 11, 136, 147T PNCS (Central star of planetary nebula) Rotational velocity/ V sin i 220, 220T, 221T Determination procedure 65 Poisson's law 122 Average rotational velocity 66, 66F Polar 366 Break-up velocity 231 Pole-on star 226, 236, 238F, 289T (Of) 216, 217T Pre-main sequence star 423,457, 477, (Oe) 219T 493F (Be) 230F, 230, 232F, 233T, 297F Profile of absorption line 58 (dMe) 325 Damping profile 58 (Red giants) 343 Doppler profile 59 (HES) 434, 436F Lorentz profile 58 (TTS) 466, 467T Voigt profile 59, 59F, 144 RS CVn stars 321,360, 361T Rotationary broaded profile 65F Runaway star 301 Propeller action 404, 405F Protostar 108, 110F, 492, 494F S Schwarzschild criterion for convection Q instability 80 Schuster-Schwarzschild model 10 R SEI method (Sobolev exct intergarion Radiation field 47, 138, 146 method) 163 Nebular type 138 Shell absorption line 166 Subject Index 525

(Be) 229,240, 241F, 242F, 256F, 257, (TTS) 458, 459F 264, 265F Spectral index (VV Cep) 360 (WR) 194, 197, 197T (HES, TTS) 487 (HES) 433 Shock wave 13, 117, 118F Spectroscopic binary Stationary shock wave 117, 118F, 119F (WR) 202, 208 Adiabatic shock wave 120, 121F (dMe) 325 Radiative shock wave 125, 126F Star cluster Shock waved in stellar atmosphere 122 Hyades' 339, 339F Shock-wave train 130 Pleiades 334, 334f, 339, 339F, 468 Shock waves in stars 122 Presepe 338, 338F (Early-type stars) 127 Orion Nebula cluster 467 (WR) 198 Star forming region (SFR) (Late-type stars) 129 (WR) 190, 193 (Mira variables) 99, 346, 348F (HES) 423 (CVs) 383 (TTS) 449, 468, 479T (HES) 433 Stark broadening 144, 144F Singular point Stark effect 60, 61 X-type 13, 89, 95, 97 Stefan-Boltzmann's law 42, 52 Alfven type 95, 96 Stellar evolution ~ Evolutionary Singular locus 91, 91F state/scenario, of stars Solar winds 87, 92 Stellar luminosity 21, 321, 323 Sound waves 117 Steller parallax 20 Sound velocity 87, 97, 117 Stellar rotation ~ Rotational velocity Generation rate of sound waves 82 Line broadening 2-41f Energy spectrum of sound waves ~ Stellar winds (theory) 13 Acoustic spectrum Coronal-type (solar type) 88F, 89, 107 Source function 44, 46, 50, 54, 178 CAK/MCAK theory 90, 91 Spectral atlas Dust driven wind 97 Atlas of representative stellar spectra Magnetic rotator model 92 (Yamashita et al.) 40 . Pulsationally driven wind 98, 100F MKK (Morgan, Keenan and Kellman) Radiation (pressure) driven wind 89, atlas 25 91F WR stars 190, 202 Wave-driven wind 100, 103F Spectral classification 3, ST Stellar wind (observation) BCD classification 25, 27F, 229, 296 (WR stars) 201, 202, 208, 210, 211 Harvard classification 6, 22, 23T (Of stars) 216, 218, 218T MK classification 24, 249 (LBV) 277 Pickering-Fleming classification 5 (P Cyg stars) 284, 285, 286F Secchi's classification 3 (Be stars) 249, 251, 254, 260 WR stars 190, 191T (B[eD 290 Of stars 215 (Binary system) 115, 116F Be stars 229, 249 (Symbiotic stars) 409 Spectral energy distribution (SED) (HES) 433, 434, 444 (Black body) 41, 42F (TTS) 453, 471, 473F (WR) 193, 194F Superionization (Be) 251, 252F (Be) 249 (HES) 427, 428F, 445 (HES) 427 (Symbiotic stars) 403 Supernova 293, 299T 526 Subject Index

Symbiotic binary 409, 410T Cataclysmic variable (CVs) 366, 366F Symbiotic novae 404, 405T, 406F Mira-type 98, 343, 344T, 350, 412 Symbiotic stars 6, 397, 398T Z Cam type 385 U Gem type = SS·Cyg type 385, T 386 Thermodynamic equilibrium (TE) ---+ TOri type 440 Equilibrium T Tau type ---+ T Tau stars Thermonuclear runaway 377, 378, 383 W UMa system 353 Transition layer 130, 323 RW Tri type 389, 391T Turbulence 62 SU UMa type 385, 389 T Tauri stars (TTS) 7, 112, 113F, 338, UX UMa type 389, 391T 448 FU Ori type (FUor) -+ FU Ori type CTTS (Classical TTS) 450, 455, 463, YY Ori type ---+ YY Ori type 468, 479 UV Cet type (flare stars) 329 WTTS (Weak-lined TTS) 450, 455, Veiling effect 262, 470 463, 468, 479 VLA (Very Large Array) 195, 403, 433 NTTS (Naked TTS) 450,480 VLBI (Very Long Baseline ETTS (Early-type TTS) 450 Interferometry) 383 PTTS (Post TTS) 450,470 V/R variation FU Ori type ---+ FU Ori type stars (Of) 218 (FUor) (Be) 259, 262, 266 yy Ori type ---+ YY Ori type stars (CVs) 387 (RES) 441 U Von Zeipel gravity darkening law 233, Ultraviolet satellite 266 IUE (International Ultraviolet Explorer) ---+ 193, 194, 201, 216, W 223, 249, 289, 321, 350, 360, 402, White dwarf companion 403F, 410, 460, 462F (WR) 206 FUSE (Far Ultraviolet Spectroscopic (Be) 300T, 301 Explorer) 350 (RS CVn) 362 Ultraviolet spectrum (CVs) 366, 375, 385, 391 (A stars) 182 (Symbiotic stars) 401, 404, 412 (WR stars) 201, 201F (Symmetric novae) 407 (Be stars) 249 Wien's displacement law 41 (Red giants) 343 Wilson-Bappu relation 7, 321, 322F, 340, (Mira) 350 340F (VV Cep) 360 Wolf-Rayet (WR) stars 5, 11, 189, 192T, (Symbiotic) 402, 403F 292 (HES) 427 [WR] star 190, 220 (TTS) 460 United Kingdom Infrared Telescope X (UKIRT) 460 X-ray binary ---+ HMXB (High-mass UXors (UX Ori type) 470 X-ray binary) X-ray satellite V ASCA (Advanced Satellite for Variable stars Cosmology and Astrophysics) 211 Hubble-Sandage variable (HS variable) Chandra satellites 329 290, 292T Einstein Observatory 197 Subject Index 527

ROSAT 182, 198, 211, 260, 431, 444, (RS CVn) 360, 361T 462 (CVs) 383 UHURU 259 (HES) 431, 444 X-ray emission/source (TTS) 462 (WR) 197 (Be) 258 y (A type stars) 182 YY Ori type/star 476, 480 (0 stars) 128 (Late-type stars) 130, 323 Z (dMe) 324F, 325 ZAMS (zero-age main sequence) 293, (Flare stars) 329 464, 492 Index of Star N arne

Stellar objects that appear only in the selected lists of respective types of stars are not included. The types of stars are indicated in the brackets in an abbreviated form after the star name. Some stars are classified into two types. Letter T or F after the page number indicates the star found in Table or Figure. The Gothic letter shows the main page of the star.

Proper name

Algol --t {3 Per Hyades cluster 339, 339F

Mira Ceti --t 0 Cet Mira B (Be/WD) 350 Orion association 337, 338F Pleiades cluster 338F, 339, 339F, 468 Pleione == 28 Tau == HD 23862 (Be) 228T, 244F, 263F, 264, 265, 265F Presepe cluster 338, 338F Rigel (B81) 3 Sirius (AI V) 3, 4T Sun 4T, 21, 62, 70, 89 Vega == Q Lyr (AO V) 3, 4T

Constellation name

A o And == HD 217675 (Be) 228T, 263F AF And (HS) 290, 292T WW And (Algol) 355F, 356 Z And == HD 221650 == MWC 416 (Symbiotic) 398, 398T, 410T Q Aql == HD 187642 (A7) 182, 183F V536 Aql (TTS) 456F V603 Aql (CN) 368T, 369 V1370 Aql (CN) 372F 1r Aqr == HD 212571 (Be) 228T, 248, 249F V 603 Aql == Aql 1918 (CN) 366, 366T, 375 Q Aur == HD 34029 (G9111) 4T E Aur == HD 31964 (Atmospheric eclipse) 356, 357T ( Aur == HD 32068 (Atmospheric eclipse) 356, 357T

529 530 Index of Star Name

AB Aur = HD 31293 (HES) 425T, 426F, 427, 428F, 430, 432F, 433T, 434, 442, 442F, 443F, 445, 446 Nova Aurigae 4 RW Aur (TTS) 7, 449T, 451F, 453, 453T, 461F SU Aur (TTS) 449T, 451F r Aur (CN) 372F UY Aur (TTS) 461F, 485F

B Q Boo = HD 124897 (K2III) 4T c Z Cam (DN) 384, 386T E Cap = HD 205637 (Be) 228T, 244F, 274 AG Car (LBV) 276F, 277 DH Car (flare) 8 S Car (Mira) 344T, 347, 349, 349T, 349F, 350 "7 Car = HD 93308 (LBV) 276, 276F, 277, 278, 278T, 279F, 280, 280F, 291, 292 , Cas = HD 5394 (Be) 4, 228T, 245T, 246, 248, 257, 257T, 258T, 259, 263F, 265, 266, 267F VX Cas (HES) 479T V376 Cas (HES) 428F V635 Cas = 4UOl15 + 634 (Be) 258T, 259 V705 Cas (CN) 375, 378F 8 Cen = HD 105435 (Be) 252F, 268, 269F J.L Cen = HD 120344 (Be) 245' CQ Cep = WR 155 = HD 214419 (WR) 209F, 210, 211T Q Cep = HD 203280 (A7) 182, 182F .A Cep = HD 210839 (Of) 218T VV Cep (Atmospheric eclipse) 357T, 357, 358F, 359, 359F AY Cet (RS CVn) 361T, 362 UV Cet (Flare) 328T, 329, 330F, 338 o Cet = HD 14386 = Mira Ceti (Mira) 4T, 98, 344T, 349F, 350, 410 SZ Cha (TTS) 488 VW Cha (TTS) 471 EZ CMa = WR 6 = HD 50896 (WR) 192T, 205T, 210 GU Cha = HD 52721 (HES) 425T, 428F Z CMa (HES, TTS, Fuor) 434, 449T, 451F, 476T w CMa = HD 56139 (Be) 245 {3 CMi = HD 58715 (Be) 228T, 245, 245T, 246 YZ CMi (Flare) 326T, 333T YZ Cnc (DN) 386T, 389, 390F, 393 R CrA (RES, TTS) 470 S CrA (TTS) 470 T CrA (TTS) 428F, 470 TY CrA (HES) 433, 425F, 437, 437T, 438 V693 CrA (CN) 372F 8 CrB = HD 141714 (gK) 320, 320F Index of Star Name 531

T CrB (RN, symbiotic) 4, 379, 379T, 380, 403 RS CVn == HD 114519 (RS CVn) 361, 361T Cyg X-3 (X-ray binary) 210 CH Cyg == HD 182917 (Symbiotic) 398T, 404 CI Cyg == MWC 415 (Symbiotic) 6,398, 398T, 399, 400F, 403 KU Cyg (Algol) 355F P Cyg == HD 193237 (LBV) 5, 276, 276F, 277, 278, 278T, 280, 282, 283F, 284 R Cyg == HD 185456 (Mira) 14 SS Cyg (DN) 386T, 386, 387F, 388, 388F, 389, 393 31 Cyg == HD 192577 (Atmospheric eclipse) 356, 357T 32 Cyg == HD 192696 (Atmospheric eclipse) 356, 357T 59 Cyg == HD 200120 (Be) 228T, 240, 241F, 263F V 444 Cyg == HD 193576 == WR 139 (WR) 192T, 209F, 210,211, 211T, 212F V 1016 Cyg (Symbiotic) 398T, 405T, 406, 406F, 407, 410T V 1057 Cyg (Fuor) 474, 475F, 476T V 1329 == HBV 475 (Symbiotic nova) 405T, 406, 406F, 407, 408F, 409F V 1331 (TTS) 461F V 1500 Cyg (Nova 1975) (CN) 368T, 369, 372F V 1515 Cyg (Fuor) 475F, 476T V 1668 Cyg (CN) 372F

D HR Del == Del 1967 (CN) 368T, 369, 406F S Dor == HD 35343 (LBV) 276F, 277, 278T, 284, 291 AG Dra (Symbiotic) 398T, 403, 403F AS Dra (RS CVn) 361 BY Dra (RS CVn) 361, 361T DR Dra (RS CVn) 331

E AQ Eri (DN) 389 RZ Eri (RS CVn) 362 A Eri == HD 33328 (Be) 270, 271F

G DN Gem == Gem 1912 (CN, Nb) 370, 371F U Gem (DN) 385, 386T YY Gem (RS CVn) 361, 361T RZ Gru (NL) 391, 391T, 392F, 393

H AD Her (Algol) 355F, 356 88 Her == HD 162732 (Be) 228T, 266 V 533 Her == Nova Her 1963 (CN) 368T, 369, 373, 373F, 374T V 775 Her == HD 175742 (RS CVn) 361 V 815 Her == HD 166181(RS CVn) 361 RW Hya == MWC 412 == HD 117970 (Symbiotic) 6,398, 398T, 4.10T TT Hya (Algol) 354F, 355 VW Hyi (DN) 386T, 389 532 Index of Star Name

L EV Lac (Flare) 328T, 331, 331F, 332, 332T, 335T EW Lac = HD 217050 (Be) 228T, 240, 244F, 263F, 270 RT Lac (RS CVn) 361T, 365 AD Leo (Flare) 328T, 331, 333F, 335T DH Leo = HD 86590 (RS CVn) 361 93 Leo (RS Cvn) 362 EX Lup (EXor) 474 GQ Lup (TTS) 488 RY Lup (TTS) 488 BF Lyn = HD 80715 (RS CVn) 361 Q Lyr --t Vega (3 Lyr = HD 174638 (Eclipsing binary) 4, 6T, 6, 300T

M (3 Man A = HD 45725 (Be) 244F AT Mic (Flare) 336 R Man (HES) 425T, 428F, 447T, 449T, 470 o Q Ori (M1 lab) 3,4T KK Oph (HES) 437T RS Oph (RN, symbiotic) 379, 379T, 380, 381F, 382, 383F, 384T, 393, 394F, 396, 398 RZ Oph (Algol) 115, 353F <" Oph (Be, Oe) 273 A Ori = HD 36861 (Of) 216T, 218T BF Ori (HES) 428F, 438 FU Ori (TTS, Fuor), 449T, 474, 475F, 476T GW Ori == HBC 85 (TTS) 449T, 468 HK Ori (HES) 425T, 447T SU Ori (TTS) 451F TOri (TTS) 425T, 426F, 438 UX Ori = HD 293762 (HES) 425T, 438, 439F, 440, 440F, 470, 479T, 490 YY Ori (TTS) 476, 477F w Ori = HD 37490 (Be, HES) 256F, 274, 425T, 428F, 488T V 380 Ori (HES) 425T, 426F, 447T

P AG Peg == HD 207757 (Symbiotic nova) 398T, 402, 405T, 406, 410T EQ Peg A (Flare) 335T I I Peg = HD 224085 (RS CVn) 366 KT Peg == HD 222317 (RS CVn) 361 AX Per == MWC 411 (Symbiotic) 6, 398, 39ST, 399, 400F, 403 KT Per (DN) 386T, 389 X Per == HD 24534 (Be) 228T, 248, 300T XY Per (HES) 437T (3 Per == Algol = HD 19356 (Algol) 115 E Per == HD 24760 (Be) 273 Index of Star Name 533

Per = HD 10516 (Be) 228T, 243, 244F, 245T, 252F, 300T 'l/J Per = HD 22192 (Be) 228T, 240, 242F, 243, 244F,245T, 257 48 Per = HD 25940 (Be) 245T, 300T RR Pic (CN) 368T, 372F 19 Pis (Carbon) 4T ( Pup = HD 66811 (04f) 75, 76, 218T NX Pup (HES) 438, 439F, 488 T Pyx (RN) 379, 379T, 380

S a Sco (M1 I) 4T S ScI (Mira) 344T, 345F, 346 AK Sco (HES) 488 U Sco (RN) 372F, 379, 379T, 380 V 856 Sco -+ HR 5999 (HES) V443 Sct (CN) 393, 394F MS Ser (RS CVn) 361 RT Ser (CN, Nc, symbiotic nova) 405T, 406 VV Ser (HES) 488 HM Sge (Symbiotic) 405T, 406, 406F, 407, 410T 9 Sge = HD 188001 (Of) 218, 218T Sgr 1991 (CN) 373F V4066 Sgr = HBC 662 (TTS) 468

T a Tau (K5III) 3 T Tau (TTS) 449T, 451F, 467T, 485F cTau = HD 37202 (Be) 228T, 242F, 243, 244F, 245T, 247, 247F, 248, 256F, 257, 257T, 265 'f} Tau = HD 23630 (Be) 228T, 245, 245T AA Tau (TTS) 455, 457F, 467T BP Tau (TTS) 451F, 467T CQ Tau (TTS) 438 CW Tau (TTS) 461F, 473, 474F DG Tau (TTS) 485F DI Tau (TTS) 467T DK Tau (TTS) 485F DN Tau (TTS) 467F DO Tau (TTS) 456F, 459F, 473 DR Tau (TTS) 461F, 472, 472F, 481, 485F DS Tau (TTS) 477F GG Tau (TTS) 459F GI Tau (TTS) 467T GK Tau (TTS) 467T HK Tau (TTS) 488 HL Tau (TTS) 456F, 485F HP Tau (TTS) 467T HV Tau (TTS) 488 IQ Tau (TTS) 459F 534 Index of Star Name

RR Tau (HES) 430, 430F, 438 RY Tau (TTS) 7, 449T, 461F, 469, 469F RW Tau (TTS) 461F, 462, 462F GK Tau (TTS) 467T GI Tau (TTS) 467T SU Tau (TTS) 467T UX Tau (TTS) 488 XZ Tau (TTS) 456F 28 Tau ---+ Pleione V410 Tau (TTS) 449T, 467T V 711 Tau == HD 22468 (RS CVn) 361, 361T, 362, 364F, 365F RR Tel (Symbiotic nova) 405T, 406, 406F

U DW UMa (NL) 391, 3919T, 392F, 393 SU UMa (DN) 386T, 390F, 396 W UMa (Eclispsing binary) 353 f3 UMi (K4III) 3 € UMi == HD 153751 (RSCVn) 361T, 362 v "'? Vel == WR 11 (WR) 192, 195,202, 203F, 205T EQ Vir (TTS) 466F HS Vir (DN) 389 W Vir (Pop. II Cep) 14 PU Vul (Symbiotic nova) 405T, 406 WW Vul (HES) 440, 441F, 479T, 480, 488

Catalogue number A0535+262 (Be) 258T, 259 BD +40°4124 (RES) 488T BD+41°3731 (HES) 428F BD +46°3471 (RES) 428F CoD -42° 11721 (RES) 486, 486F CoD -44°3318 (HES) 488T CPD-52°9243 (LBV) 287 Elias 1 (HES) 434 Elias 12 (TTS) 482F ESO Ha 28 (RES) 488 GL 388 == AD Leo (dMe) 326F GL 487 (dMe) 326F GL 490a == BF CVn (dMe) 326F GL 490b (dMe) 326F GL 494 == DT Vir (dMe) 326F GL 616-2 == CR Dra (dMe) 326F GL 644a,b (dMe) 326F GL 669 a,b (dMe) 326F HBC 85 ---+ GW Ori (TTS) Index of Star Name 535

HBC 662 ~ V4066 Sgr (TTS) HD 4004 = WR1 (WR) 129T, 201 HD 5005 (Of) 217F HD 5394 ~ "I Cas (Be) HD 9974 = WR 3 (WR) 192T, 198, 200F HD 10516 ~ ¢ Per (Be) HD 14386 ~ 0 Cet (Mira) HD 15558 (Of) 218T HD 15570 (Of) 216, 217F, 218T HD 16523 = WR 4 (WR) 192T, 214T HD 19356 ~ {3 Per (Algol) HD 22192 ~ 1jJPer (Be) HD 22468 -+ V 711 Tau (RS CVn) HD 23862 ~ 28 Tau (Be) HD 24534 ~ X Per (Be) HD 31293 ~ AB Aur (HES) HD 31648 (B[eD 275T HD 31964 ~ e Aur (Atmospheric eclipse) HD 32068 ~ ( Aur (Stmospheric eclipse) HD 35343 ~ S Dra (LBV) HD 35929 (HES) 432F, 433T HD 37202 ~ ( Tau (Be) HD 37490 ~ w Ori (Be, HES) HD 39680 (Oe) 219, 219T HD 41335 (Be) 256F HD 44458 (Be) 256F HD 45677 = FS CMa (Be) 274, 275T HD 50138 (B[eD 275T HD 50896 = WR 6 ~ EZ CMa (WR) HD 51585 (B[eD 275T HD 52721 ~ GU CMa (HES) HD 53367 (HES) 438 HD 58647 (HES) 432F, 433T HD 66811 -+ ( Pup (Of) HD 68273 = WR 11 ~ "12 Vel HD 79573 = WR 15 (WR) 214T HD 70309B (TTS) 471 HD 73974 (gK) 320, 320F HD 86161 = WR 16 (WR) 205T, 214T HD 92740 = WR 22 (WR) 208,209, 209F HD 93308 ~ "7 Car (LBV) HD 96548 = WR 40 (WR) 205T, 214T HD 100546 (Ae) 183 HD 104994 = WR 46 (WR) 205, 205T, 206, 206F HD 105435 ~ 8 Cen (Be) HD 117297 = WR 53 199F HD 117970 ~ RW Hya (Symbiotic star) HD 141569 (HES) 437T HD 144668 ~ HR 5999 (HES) 536 Index of Star Name

HD 149757 --* ( Oph (Oe, Be) HD 150193 (HES) 437T, 488T HD 151932 = WR 78 (WR) 198, 214T HD 158860 = WR 94 (WR) 199F HD 163296 (B[e], HES) 275T, 488T HD 165688 = WR 111 (WR) 192T, 198, 214T HD 167362 (B[eD 275T HD 168076 (Of) 217T HD 174638 --* {3 Lyr (Eclipsing binary) HD 177230 = WR 123 (WR) 205T, 213, 214T HD 182917 --* CH Cyg (Symbiotic) HD 188001 --* 9 Sge (Of) HD 191765 = WR 134 (WR) 4, 162F, 192T, 201, 213 HD 192103 = WR 135 (WR) 5, 192T, 207, 207F HD 192163 = WR 136 (WR) 162F, 192T, 198, 200F, 201, 205T HD 192641 = WR 137 (WR) 5, 192T, 202, 204F HD 193237 --* P Cyg (LBV) HD 193576 = WR 139 --* V444 Cyg (WR) HD 193793 = WR 140 (WR) 192T, 194, 194F, 202, 204F, 205 HD 193928 = WR 141 (WR) 192T, 201 HD 197406 = WR 148 (WR) 192T, 210 HD 200120 --* 59 Cyg (Be) HD 200775 = MWC 361 (HES) 437T, 480T, 483, 488T HD 207757 --* AG Peg (Symbiotic) HD 214410 = WR 155 --* CQ Cep HD 217050 ~ EW Lac (Be) HD 221650 --* Z And (Symbiotic) HD 250550 (HES) 438 He2-131 (PNN) 222, 223F HenS 12 ([BeD 287T, 289T HenS 22 (B[eD 287T, 289, 289T HenS 134 ([BeD 287T, 289T HH 30 (TTS) 488 HH 105 (HH obiect) 447 HR 4621 (Be) --* 8 Cen HR 5999 = HD 144668 = V856 Sco (HES) 425T, 426F, 427,438, 439F, 488, 488T HR 7574 --* 9 Sge (Of) IC 348 (star cluster) 468 L726-8 (Flare) 8 Lalande 21258B (Flare) 8 LkHa 198 (HES) 447T LkHa 234 (HES) 447, 447T, 448F LSS 3013 --* WR 50 (WR) M31 (Andromeda Galaxy) 290, 291F, 292 M33 (Galaxy) 290, 291F, 292 MWC 300 (LBV, HES) 287, 434 MWC 314 (B[eD 290 MWC 349 (B[eD 275T, 290 MWC 361 (HES) 432F, 433T Index of Star Name 537

MWC 411 -t AX Per (Symbiotic) MWC 412 -t RW Hya (Symbiotic) MWC 415 -t CI Cyg (Symbiotic) MWC 416 -t Z And (Symbiotic) MWC 480 (HES) 432F, 433T MWC 645 (B[eD 275T MWC 1080 (HES) 425T, 432F, 433T, 437T, 447T, 486 NGe 2264 (star cluster) 338, 338F NGC 3766 (star cluster) 296, 297F NGC 4755 (star cluster) 296, 296F NGC 7000 (star cluster) 338F NGC 7027 (PN) 221 NGC 7129 (refl. Nebula) 447 R 50 (B[eD 287T, 287, 288F, 289, 289T R 66 (B[eD 287T, 289T R 82 (B[eD 287T, 289, 289T R 126 (B[eD 287T, 289T Star No, 103 in Pleiades (slow flare) 334, 334F Sz 06, 19, 62, 65, 68, 77, 82, 98 (TTS) 466F 4UOl15+634 -t V635 Cas WR 50 = LSS 3013 (WR) 205T WR 56 = LSS 3117 (WR) 214T WR 116 (WR) = AS 306 (WR) 199F WR 124 (WR) 214T WR 125 (WR) 204F WR 156 (WR) 214T