INDEX of NAMES Aarseth, S.J., 59, 640 Abell, G.O., 24, 26, 41, 334

Total Page:16

File Type:pdf, Size:1020Kb

INDEX of NAMES Aarseth, S.J., 59, 640 Abell, G.O., 24, 26, 41, 334 INDEX OF NAMES Aarseth, S.J., 59, 640 Baan, W.A., 461-46 ...~bl:;ott, I::: .. c., 98, llJ BahcctJJ, J.N*~ 6, , 422; 4J3 Abell, G.O., 24, 26, 41, 334, Bailey, J., 483, 4 6 550, 556, 572 Baity, W.A., 169, 7 Abramowicz, M.A., 113-114, Balbus, S.A., 108, 1 0 117-118, 126, 447, 507, 543, Bald\...Jin,. J .. A~ , 1 q, 2 , 29, 34. ::.46 39, 41~42. 60, 110, 195, 193, Achterberg, A., 522-523 )08, 210, 370~ 4JJ. ~~zs·-~~26 .. Adam, G., 42, 272 529, ~177 Adams. M.T., 637, 640 Ba.l i c k ,. B . ,. 2 l £ 41 ,. 4 9 I 59 , Adams, T.F., 207-208, 689, 692 250, 270, 312-313 Ade, F.A.R., 19 Balkowski, C., 502 Aguirre, C., 271 Balzano, V .."A.., 196, 208, 210, Aharonian, F .A., 151, lf:.9 216.- 225,. 73~S Ahmed , F. , 57 7 Barbieri, C., 82, 87, 0-91, Ak.hiezer, A. I .. , r-")22-523 340, 350, 46~, 601-6 3 Aldrovandi, S.M.V., 476-477 Bardeen, J., 96, 110, 85, 39J Alladin, S.M., 573, 577 Barr ,. P . ,. 9 1 , 52 8 - 5 2 9 ,. b b 9 - 6 7 0 Allen, C.W., 645, 647 Barrow, J.D., 555, 558 Allen, D.A., 77, 582 Bar·tel. N. ,- 653 Aller, H.D., 77, 653 Barthel, F.D .• 568 Aller, M.F., 77, 653 Bassani, L .• 727, 735 Allain. D., 341, 349, 672 Baud , B , , 2 7 0 Altamore, A .• 275 Bauer, E., 661 Altschuler, D.R., 655, 657 Baum, W.A., 577 Ambartsumian, V.A., 132, 143, Beck, S.C .. 634-635 586 Becker, R.H., 269-271 Anderson, K.S., 707-708 B~cklin, E.E., 19, 42, Andrew, B.H., 87, 90-91 :.~86 f 63:.; ··636 Angel, J.R.P., 64, 77-79, 87, Beckman, J.E .• 471-472, 474, 91, 246, 250 587, 591, 601, 604 Antonucci, R.R.J., 669 Beckwith, S., 534-6351 725 Arakelian, M.A., 258, 269 Begelman, M.C., 130, lJ4, Arp, H. C. , 54-55, 59, 26£., 46 7, 142-143, 150, 169, 448, 45J, 470, 574, 577, 618 455, 521. 523, 717, 721 Athana:~soula, E., 640 Beichman, C.A., 19, 270-271 Atherton, P.D., 304 Beintema, D.A., 270-271 Atwood, B., 422, 432-433 Bet·geron, J. , 42, ~59, 300, 304, Aumann, H.H., 270-271 421-423. 425-426, 429, 433-434 Auriemma, C., 439, 441, 698, Bertola, F., 176, 190, 299, 700, 702, 704 302' 304 Aveni, A.F., 677 Bettoni, D., J04 Avni, Y., 6, 8, 226, 237, 242, Bhattachat-ia, D., 501-502 250, 334, 350, 337, 399-411, Bhavsar, S.P., 555, 558 413-414, 416, 418-413, 494, Bicknell, G.V., 541 540, 547-548, 550, 632 Biermann, P., 77, 248, 251, Avrett, E.H., 681 303-304, 552, 554, 618 Axford,, W.I., 140, 143 Bignami, G.F., 150, 168-169 Axon, D.J., 304, 483, 486, 652 Binette, L., 37, 41, 200, 208, 259, 269, 305, 475-477, 704 Baade, D .. , 554 Bingelli,, 181 741 742 INDEX OF NAMES Bingham, R.G., 649, ~52 Brand, F.W.J.L., 484, 486 Bir·etta, J., 41, 543, S46 Branduardi, G., 269, 419 BirklC?, K, 479 Beecher, K., 681 Bjornsson, C.-I., 483, 521, 523 Breqman, J.N., 16-17, 19, 77, Blackman, C.P .• 26, 41 534-·535' 735 Blad,~:,, ,J.C., 77, ~':7<), 425-426, Bridle, A., 52, 59, 304, 439, 4:13 441, 565, ~68, GJ9-640, 717, HlaP.:.:;, O~IV1,, 1.13-·114, 119, 1.21, 721 123-124, 126 Bf·iel, U., 269 Blake. G.M., 510-511 Briggs, F.H., 428, 433 Blanco, V. M., 269 Brinkman, W., 270-271, 455, Bland, J., 302, 304 523.: SjO Blandford, R.D., 75, 77, lOH, Erinkmann, W., l~l 110, 114. 124, 126, 143, 1'30, Rrumage, G.E., 144, 275, 291 1~2. 163, 166. 169, 246, 250, Rr.ord.{~tlla, IA1~, b49. t;51··652 4 4 8 I' 4-5 ~.i 1 >11 f ~i 2 l ,. 52 3 1 54 4 ; Bros~he, 2., 49S 500, 502 546 Rt·owne~ 1~W .. A., 461,470, 62:i, Bleach, R.D., 271 E.~~ b Blumenthal, G.R., 1W3-190, Bruc ~<, H. A. , 2 :::~ l 778-729. 735 Br·Ltyn,. 671 Buernstein, L., 694 Bnnual, G., 176--177, 180, 190 Bog<.Je~~,;. A., 2'26, 514, 516 Buitrago, J., ~03-50~, 507 BoggPss, N., 270-271 Bujdrrabal, V., 500, 502 Bohlin. R.C., 513, 516 BurbiJge, E.M., 19, 48, 55-56, Bohuski. T.J., 256, 269 59-60, 475, •P7 Bois:o;e, P., 422, 42::,, 433 Burbidge, G., 47-48, 50, 54-56, Boksenberg, A., 42, 143-144, 59, 77, 81, 91, 475, 477 275, 298, 304, 434, 546, 716 Burke, W.~., 370 Boldl, E.A., 269·271, 383--385, Burns, M.L., 1~51, 169 387, 189-39!, 393 394 Bul~her, H .. 304 Bolton, ,J.B., 467, 47C: Butcher, H.R., 41, 298, 304 Bu 1 t. GI1 , ,] • G . , 7 '3 , ~; l ~/ , ~·\ 1 '?I Byard, P.L., 482 Bondi, H., 117, 122, 126 Byram, E.T., 272 Bono1i, C., 487-488 Boned i, F'., 82, 84 -s:., 91, :1:34, Callan, C., G61, 667 350, 487, 502, 631 Calucci, G .. 667 Borc•son, T.A., 18--l'), 21, 41, ~alvani, M., ~46 4 •J • 59 • 2 3 9 I J Ci •t ' :H l . 3 lJ Cam~nzind, M., 476-477, 521, 523 Borto1etLo, F., 487-488 Cameron, A.G.W., 139, 143 Bosma, A., 707-708 Campbell, B., 42, 59, 312-313, Bothun, G.D., 59, 250, 312-313, 554, 608 642, 644 Canizares, C., 269 Bottinel1i, L., 501-502, 622 Canizares, C.R., 215, 226, 270, Bc•uchet, P. , 91 299, 304, 399, 403, 418 Bowy€!t··, C.S., 271 Canizares, R.G., 249-250, 547, Bowyer, S., 42, 77 5~50 Boy 1 e , B . J • , 2 3 2 , 2 50 , 3 2 5 , Cannon, R.D., 82, 91, 582 346, 350, 412, 418, 491-493, Capaccioli, M., 176, 190, 269, 631 350 Braccesi, A., 85, 91, 224-226, Carroll, T.J., 40-41, 509-511 239, 250, 317, 319, 325, 334, Carswell, R.F., 78, 425, 433-434 339, 341, 346-347, 349-350, Carter, D., 204, 208, 266, 269, 365, 370, 403, 405, 412, 419, 271, 302, 304 494, 502, 540, 631-632 Cassatella, A., 513, 516, 709 Bracewell, R.N., 91 Castor, J.I., 98, 110 INDEX Of NAMES 743 81 91 f L···,, Ct-ctmpton, Li~, 42, ::..1:t • .3lJ ~ 5:54, 2 ~:: ~-~ ' 2 3 l -- 2 2 ~ 24 I 2=lo,. 608 3JJ 1 J£,1 f ~'' 4 2, 418, Crane, P.C., 270 -':._.. Crenshaw, D.M., 48 Cav~:.:-l_llc;, G .• 5' '33 C r· i ::; t: ian i. , :_) . , 8l • e ~J , ·:-~ 0 ~ '3 J Ch.affee 1 F .. H., 4l2-43J 350,. 46~;, 470 Chanan, G.A., 21, 42, 59, 69, C r:· C)n1\..Je l ·L , E .. H . J 7 0 2 , 7 0 •J Cruz-Gunzales, ~., 78, 483, 4BA Char·leb. P ~A., 22 1 4;2 ~ 1.9~~; ~10 Cudworth, K.M., 117, 320, 334 Cheney. J., 451, 455 Cunnjfft!, F'.l::., 298, JCJ4 20:] F :23~5 t 2~~,0 F 264 f 268 --2691 I)' Addi.l:r- ~L o ..- R ~ , {~.4 0 126-327, 330-332, 134, D' Al~ssandrc), !'"1 .. ~ 487·-488 539-540, 548, 550, 202, ,-,., r. 631, t2i43-C44 207~2C8, £..J...U1 241. if"/5 T Chenq, F. H., 583 "'i ") -, ChPster. T.J., 19 Danese. L., 41, 208, 226, .£. ••••.··. f Chiavpet i. L., 9L !::. ""1-, Cl-Lincar·:i.n.i ~- G., :_:.~;4, :.. ..'! L Ch.iu,. L~-T~G .. , Jl7,. 320~ 6J.i, C44 3:;:::~ -- 32(:, 1" 334 f "340 1 J:;o 1 :370 Ddnielson, R. F:., l42--l4J Christiansen, W., 510-511 Dan z i <:p:? r , I ... J ~ , 8 , ::-~ 2 , 59 ,. 7 8 .­ 1 ::=~17--51:1 Chui Y. '31 0 2 6 9 ~ 2 71 ~ 2 9 8- 3 0 0 F ~1 0 2 1 Chubb, T.A., 272 304, 350, 418, 618, 676-677 Ciardullo, R., 59 Davidson. K .. , 9-/, 106, 110,_ ~iur·la, T'., 604 531, 535 Clark, G~ .- 263 I:ia V :i S , M • , 3 3 ,. 4 l , 1 9 :-_; , 2 0 9 ,. Cl::..n.rr:?l I J. , 144 ~" 275, :?90 70'3 350, 441, 482, 519, 568, Clr.:~t~:J, P.E.~ 16, 13, 270·-- 71 62B. -62{3 I 632 C l uv;e s , R . G. , 3 4 0 , 3 50 • 4 • , de Bruyn, A.G~, 642, 644 469 470, 493-494, 631 dt"? Grijp,. M~H.K. J 14, 19, 204, Cnuvaev, K.K., 672 208, 2G6-268, 270, 608 Cc,fu::-n, M.f-L~ 52~ ~~9--60, 31, 91, dt! JontJ,. T., 19, 204f 208,. 270, lOt~, llO ~~07 It 608 Cohen, R.D., 669. 671 De Rubertis, M., 241, 250 Cohn I H ~ , l :12 --13 3 ~ 13 ':i -- 14 0 . 14 3 DeRobertis, M.M., 33, 41, 204, Coleman, C~.S .. 1 511,521, ~~23 208 Coleman, G.D., 217, 225 de Vaucou1eurs, A., 23, 41, 271 Colgate, S.A., 140, 142~143 de Vaucou1eurs, G., 23, 11, Colina, L., 525, 528 271, ~i£)2 i 5801 582 Collin,, 42'3 de Young, D., 54, 59 Collin~Souffrin, ......c 531-532, IJe Zotti, G., 41, 208, 226, 535 232, 250, 263, 334, 384, 394, Cominsky, L., 269 418, 488, 514, 516, 537, 540, Condon, J.J., 18-19, 91, 329, 548, 550, 631, 644 334, 41'3, 441, 467, 470, 566, Dean, A.J., 727, 735 568 Deemimg, T.J., 589-590, 603-604 Contini, M., 476-477 Dehari, 0., 49, 59 Cooke, B.A., 264, 269 Dekel, A., 186, 190 Corwin, H.G.Jr., 23, 41, 271 Delpino, F., 487 Couch, W.J., 177, 190 Delvaille, J.P., 271 Courvoisier, T.J.-L., 476-477 Demoulin-Ulrich, M.H., 298, 304 Coyne, G.V., 251, 486 Dennefeld, M., 266, 269, 304 Craine, E.R., 474 Dewitt, B., 455 744 INDEX OF NAMES Dewitt, C.
Recommended publications
  • On the Origin and Propagation of Ultra-High Energy Cosmic Rays (Measurements & Prediction Techniques)
    Dissertation On the Origin and Propagation of Ultra-High Energy Cosmic Rays (Measurements & Prediction Techniques) Nils Nierstenhoefer Wuppertal, 2011 University of Wuppertal Supervisor/First reviewer: Prof. Dr. K.-H. Kampert Second reviewer: Prof. Dr. M. Risse Motivation & Preface It is a long known fact that cosmic rays reach Earth with tremendous energies of even above 1020 eV. Despite of decades of intensive research, it was not possible to finally reveal the origin of these par- ticles. The main obstacle in this field is their rare occurrence. This is due to a very steep energy spectrum. To make this point more clear, one roughly expects to observe less than one particle per km2 in one century exceeding energies larger than 1020 eV. To overcome the limitation of low statis- tics, larger and larger cosmic ray detectors have been deployed. Today’s largest cosmic ray detector is the Pierre Auger observatory (PAO) which was constructed in the Pampa Amarilla in Argentina. It covers an area of 3000 km2 and provides the largest set of observations of ultra-high energy cosmic rays (UHECR) in history. A second difficulty in understanding the origin of UHECR should be pointed out: Galactic and extra- galactic magnetic fields might alter the direction of even the highest energy events in a way that they do not point back to their source. In 2007 and 2008, already before the completion of the full detector, the Auger collaboration pub- lished a set of three important papers [1, 2, 3]. The first paper dealt with the correlation of the arrival directions of the highest energetic events with the distribution of active galactic nuclei (AGN) closer than 75Mpc from a catalog compiled by Veron-Cetty and Veron (VC-V) [4].
    [Show full text]
  • Hot Interstellar Matter in Elliptical Galaxies
    Hot Interstellar Matter in Elliptical Galaxies For further volumes: http://www.springer.com/series/5664 Astrophysics and Space Science Library EDITORIAL BOARD Chairman W. B. BURTON, National Radio Astronomy Observatory, Charlottesville, Virginia, U.S.A. ([email protected]); University of Leiden, The Netherlands ([email protected]) F. BERTOLA, University of Padua, Italy J. P. CASSINELLI, University of Wisconsin, Madison, U.S.A. C. J. CESARSKY, Commission for Atomic Energy, Saclay, France P. EHRENFREUND, Leiden University, The Netherlands O. ENGVOLD, University of Oslo, Norway A. HECK, Strasbourg Astronomical Observatory, France E. P. J. VAN DEN HEUVEL, University of Amsterdam, The Netherlands V. M. KASPI, McGill University, Montreal, Canada J. M. E. KUIJPERS, University of Nijmegen, The Netherlands H. VAN DER LAAN, University of Utrecht, The Netherlands P. G. MURDIN, Institute of Astronomy, Cambridge, UK F. PACINI, Istituto Astronomia Arcetri, Firenze, Italy V. RADHAKRISHNAN, Raman Research Institute, Bangalore, India B . V. S O M OV, Astronomical Institute, Moscow State University, Russia R. A. SUNYAEV, Space Research Institute, Moscow, Russia Dong-Woo Kim Silvia Pellegrini Editors Hot Interstellar Matter in Elliptical Galaxies 123 Editors Dong-Woo Kim Harvard Smithsonian Center for Astrophysics Garden Street 60 02138 Cambridge Massachusetts USA [email protected] Silvia Pellegrini Dipartimento di Astronomia Universita` di Bologna Via Ranzani 1 40127 Bologna Italy [email protected] Cover figure: Chandra image of NGC 7619. From Kim et al. (2008). Reproduced by permission of the AAS. ISSN 0067-0057 ISBN 978-1-4614-0579-5 e-ISBN 978-1-4614-0580-1 DOI 10.1007/978-1-4614-0580-1 Springer Heidelberg Dordrecht London New York Library of Congress Control Number: 2011938147 c Springer Science+Business Media, LLC 2012 This work is subject to copyright.
    [Show full text]
  • A Search for Transiting Extrasolar Planets in the Open Cluster NGC 4755
    ResearchOnline@JCU This file is part of the following reference: Jayawardene, Bandupriya S. (2015) A search for transiting extrasolar planets in the open cluster NGC 4755. DAstron thesis, James Cook University. Access to this file is available from: http://researchonline.jcu.edu.au/41511/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://researchonline.jcu.edu.au/41511/ A SEARCH FOR TRANSITING EXTRASOLAR PLANETS IN THE OPEN CLUSTER NGC 4755 by Bandupriya S. Jayawardene A thesis submitted in satisfaction of the requirements for the degree of Doctor of Astronomy in the Faculty of Science, Technology and Engineering June 2015 James Cook University Townsville - Australia i STATEMENT OF ACCESS I the undersigned, author of this work, understand that James Cook University will make this thesis available for use within the University Library and, via the Australian Digital Thesis network, for use elsewhere. I understand that, as an unpublished work, a thesis has significant protection under the Copyright Act and; I do not wish to place any further restriction on access to this work. 2 STATEMENT OF SOURCES DECLARATION I declare that this thesis is my own work and has not been submitted in any form for another degree or diploma at any University or other institution of tertiary education. Information derived from the published or unpublished work of others has been acknowledged in the text and list of references is given.
    [Show full text]
  • Mass Distribution in Galaxy Clusters
    Pontificia Universidad Cat´olicade Chile Facultad de F´ısica Instituto de Astrof´ısica The Blue Straggler Star Populations in Galactic Globular Clusters by Mirko Simunovic Mu~noz Thesis presented to the Instituto de Astrof´ısica, Facultad de F´ısica, Pontificia Universidad Cat´olica de Chile to obtain the degree of Doctor in Astrophysics Thesis presented to the Combined Faculties for the Natural Sciences and for Mathematics of the Ruperto-Carola University of Heidelberg, Germany to obtain the degree of Doctor of Natural Sciences Supervisors : Prof. Dr. Thomas H. Puzia Prof. Dr. Eva K. Grebel Correctors : Prof. Dr. Marcio Catel´an Prof. Dr. Dante Minnitti Prof. Dr. Jorge Alfaro Santiago − Heidelberg 2016 Dissertation submitted to the Instituto de Astrof´ısica,Facultad de F´ısica Pontificia Universidad Cat´olicade Chile, Chile for the degree of Doctor in Astrophysics submitted to the Combined Faculties for the Natural Sciences and for Mathematics of the Ruperto-Carola University of Heidelberg, Germany for the degree of Doctor of Natural Sciences Put forward by Mirko Simunovic Mu~noz born in: Antofagasta, Chile Oral examination: October 19, 2016 The Blue Straggler Star Populations in Galactic Globular Clusters Mirko Simunovic Mu~noz Astronomisches Rechen-Institut Referees: Prof. Dr. Eva K. Grebel Prof. Dr. Thomas H. Puzia vi Abstract The puzzling existence of Blue Straggler Stars (BSSs) implies that they must form in relatively recent events, after the majority of the constituent globular cluster (GC) stellar population was formed. In this thesis we compile a large set of independent work to help understand the formation of BSSs. In Chapter2 we present new proper-motion cleaned BSS catalogs in 38 Milky Way GCs based on multi-passband and multi-epoch treasury survey data from the Hubble Space Telescope.
    [Show full text]
  • April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
    Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86.
    [Show full text]
  • OBSERVING GALAXIES in ANDROMEDA As You Look Towards
    OBSERVING GALAXIES IN ANDROMEDA As you look towards Andromeda you are looking out into deep space underneath the Perseus spiral arm of our milky way. The constellation has a good density of observable galaxies. There is a group of relatively local galaxies which are less than 20 million light years away and then a big gap to the rest which are over 200 million light years away. The constellation is well place from late summer to mid-winter. M31 / M32 / M110 These galaxies are generally the first galaxies that amateur astronomers observe first. M31 is visible to the naked eye in dark skies. M31 whilst bright and large is fairly bland in appearance until you start to look a bit closer. With good conditions, the dark line of a dust lane is visible. I have to say that observing two of the globular clusters of this galaxy rank up there in my most memorable observations ever. M32 is very bright and I have seen it in binoculars as a very small bright blob. M110 can be a challenge to see with its low surface brightness. Having said that, I have seen it easily in my 80mm binoculars when the sky was transparent. NGC404 This galaxy is memorable to observe as it is close to the star Mirach and hence is known as Mirach’s ghost. It is a lovely circular low surface brightness glow that is visible with direct vision in my 10 inch reflector and was visible at low power with averted vision even with Mirach in the field of view.
    [Show full text]
  • 7.5 X 11.5.Threelines.P65
    Cambridge University Press 978-0-521-19267-5 - Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer’s New General Catalogue Wolfgang Steinicke Index More information Name index The dates of birth and death, if available, for all 545 people (astronomers, telescope makers etc.) listed here are given. The data are mainly taken from the standard work Biographischer Index der Astronomie (Dick, Brüggenthies 2005). Some information has been added by the author (this especially concerns living twentieth-century astronomers). Members of the families of Dreyer, Lord Rosse and other astronomers (as mentioned in the text) are not listed. For obituaries see the references; compare also the compilations presented by Newcomb–Engelmann (Kempf 1911), Mädler (1873), Bode (1813) and Rudolf Wolf (1890). Markings: bold = portrait; underline = short biography. Abbe, Cleveland (1838–1916), 222–23, As-Sufi, Abd-al-Rahman (903–986), 164, 183, 229, 256, 271, 295, 338–42, 466 15–16, 167, 441–42, 446, 449–50, 455, 344, 346, 348, 360, 364, 367, 369, 393, Abell, George Ogden (1927–1983), 47, 475, 516 395, 395, 396–404, 406, 410, 415, 248 Austin, Edward P. (1843–1906), 6, 82, 423–24, 436, 441, 446, 448, 450, 455, Abbott, Francis Preserved (1799–1883), 335, 337, 446, 450 458–59, 461–63, 470, 477, 481, 483, 517–19 Auwers, Georg Friedrich Julius Arthur v. 505–11, 513–14, 517, 520, 526, 533, Abney, William (1843–1920), 360 (1838–1915), 7, 10, 12, 14–15, 26–27, 540–42, 548–61 Adams, John Couch (1819–1892), 122, 47, 50–51, 61, 65, 68–69, 88, 92–93,
    [Show full text]
  • Brightness Profiles of Early-Type Galaxies Hosting Seyfert Nuclei
    A&A 469, 75–88 (2007) Astronomy DOI: 10.1051/0004-6361:20066684 & c ESO 2007 Astrophysics The host galaxy/AGN connection Brightness profiles of early-type galaxies hosting Seyfert nuclei A. Capetti and B. Balmaverde INAF - Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy e-mail: [capetti;balmaverde]@oato.inaf.it Received 2 November 2006 / Accepted 15 March 2007 ABSTRACT We recently presented evidence of a connection between the brightness profiles of nearby early-type galaxies and the properties of the AGN they host. The radio loudness of the AGN appears to be univocally related to the host’s brightness profile: radio-loud nuclei are only hosted by “core” galaxies while radio-quiet AGN are only found in “power-law” galaxies. We extend our analysis here to a −1 sample of 42 nearby (Vrec < 7000 km s ) Seyfert galaxies hosted by early-type galaxies. From the nuclear point of view, they show a large deficit of radio emission (at a given X-ray or narrow line luminosity) with respect to radio-loud AGN, conforming with their identification as radio-quiet AGN. We used the available HST images to study their brightness profiles. Having excluded complex and highly nucleated galaxies, in the remaining 16 objects the brightness profiles can be successfully modeled with a Nuker law with a steep nuclear cusp characteristic of “power-law” galaxies (with logarithmic slope γ = 0.51−1.07). This result is what is expected for these radio-quiet AGN based on our previous findings, thus extending the validity of the connection between brightness profile and radio loudness to AGN of a far higher luminosity.
    [Show full text]
  • Making a Sky Atlas
    Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it.
    [Show full text]
  • Ngc Catalogue Ngc Catalogue
    NGC CATALOGUE NGC CATALOGUE 1 NGC CATALOGUE Object # Common Name Type Constellation Magnitude RA Dec NGC 1 - Galaxy Pegasus 12.9 00:07:16 27:42:32 NGC 2 - Galaxy Pegasus 14.2 00:07:17 27:40:43 NGC 3 - Galaxy Pisces 13.3 00:07:17 08:18:05 NGC 4 - Galaxy Pisces 15.8 00:07:24 08:22:26 NGC 5 - Galaxy Andromeda 13.3 00:07:49 35:21:46 NGC 6 NGC 20 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 7 - Galaxy Sculptor 13.9 00:08:21 -29:54:59 NGC 8 - Double Star Pegasus - 00:08:45 23:50:19 NGC 9 - Galaxy Pegasus 13.5 00:08:54 23:49:04 NGC 10 - Galaxy Sculptor 12.5 00:08:34 -33:51:28 NGC 11 - Galaxy Andromeda 13.7 00:08:42 37:26:53 NGC 12 - Galaxy Pisces 13.1 00:08:45 04:36:44 NGC 13 - Galaxy Andromeda 13.2 00:08:48 33:25:59 NGC 14 - Galaxy Pegasus 12.1 00:08:46 15:48:57 NGC 15 - Galaxy Pegasus 13.8 00:09:02 21:37:30 NGC 16 - Galaxy Pegasus 12.0 00:09:04 27:43:48 NGC 17 NGC 34 Galaxy Cetus 14.4 00:11:07 -12:06:28 NGC 18 - Double Star Pegasus - 00:09:23 27:43:56 NGC 19 - Galaxy Andromeda 13.3 00:10:41 32:58:58 NGC 20 See NGC 6 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 21 NGC 29 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 22 - Galaxy Pegasus 13.6 00:09:48 27:49:58 NGC 23 - Galaxy Pegasus 12.0 00:09:53 25:55:26 NGC 24 - Galaxy Sculptor 11.6 00:09:56 -24:57:52 NGC 25 - Galaxy Phoenix 13.0 00:09:59 -57:01:13 NGC 26 - Galaxy Pegasus 12.9 00:10:26 25:49:56 NGC 27 - Galaxy Andromeda 13.5 00:10:33 28:59:49 NGC 28 - Galaxy Phoenix 13.8 00:10:25 -56:59:20 NGC 29 See NGC 21 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 30 - Double Star Pegasus - 00:10:51 21:58:39
    [Show full text]
  • Prevalence of Tidal Interactions Among Local Seyfert Galaxies
    To be submitted to the Astrophysical Journal Preprint typeset using LATEX style emulateapj v. 04/21/05 PREVALENCE OF TIDAL INTERACTIONS AMONG LOCAL SEYFERT GALAXIES Cheng-Yu Kuo1,3 Institute of Astronomy & Astrophysics, Academia Sinica, PO Box 23-141, Taipei 10617, Taiwan Department of Astronomy, University of Virginia, Charlottesville, VA 22904 Jeremy Lim Institute of Astronomy & Astrophysics, Academia Sinica, PO Box 23-141, Taipei 10617, Taiwan Ya-Wen Tang1,2 Institute of Astronomy & Astrophysics, Academia Sinica, PO Box 23-141, Taipei 10617, Taiwan Department of Physics, National Taiwan University, No. 1, Sec. 4, Roosevelt Rd., Taipei 106, Taiwan and Paul T. P. Ho1,4 Institute of Astronomy & Astrophysics, Academia Sinica, PO Box 23-141, Taipei 10617, Taiwan Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 To be submitted to the Astrophysical Journal ABSTRACT No mechanisms have hitherto been conclusively demonstrated to be responsible for initiating optically-luminous nuclear (Seyfert) activity in local disk galaxies. Only a small minority of such galax- ies are visibly disturbed in optical starlight, with the observed disturbances being at best marginally stronger than those found in matched samples of inactive galaxies. Here, we report the first system- atic study of an optically-selected sample of twenty-three active galaxies in atomic hydrogen (HI) gas, which is the most sensitive and enduring tracer known of tidal interactions. Eighteen of these galaxies are (generally) classified as Seyferts, with over half (and perhaps all) having [OIII] luminosities within two orders of magnitude of Quasi-Stellar Objects. Only ∼28% of these Seyfert galaxies are visibly dis- turbed in optical DSS2 images.
    [Show full text]
  • Publications of Richard W. Pogge
    Publications Richard William Pogge Updated: 2021 March 10 Doctoral Dissertation “The Circumnuclear Environment of Nearby, Non-Interacting Seyfert Galaxies”, University of California, Santa Cruz, June 1988. (Abstract published in PASP, 100, 1296, 1988. See also #7, 8, 10, 11, & 12 below.) Papers Published in Peer-RevieWed Journals 1. “X-Ray, Radio, and Infrared Observations of the Rapid Burster (MXB 1730-335) During 1979 and 1980”, LaWrence, A., et al. (52 authors), 1983, ApJ, 267, 301 2. “The Spectra of Narrow-Line Seyfert 1 Galaxies”, Osterbrock, Donald E., & Pogge, Richard W. 1985, ApJ, 297, 166 3. “The Extended Narrow Emission-Line Region of NGC 7469 Revisited”, DeRobertis, M.M. Pogge, R.W. 1986, AJ, 91, 1026 4. “Star Forming Regions in Gas-Rich Lenticulars. I. Ha Imaging of an Initial Sample of Galaxies”, Pogge, Richard W., & Eskridge, Paul B. 1987, AJ, 93, 291 5. “FY Aquilae and the Gamma-Ray Burst Event of 1979 March 31”, Hartmann, Dieter, & Pogge, Richard W. 1987, ApJ, 318, 363 6. “Optical Spectra of Narrow Emission Line Palomar-Green Galaxies”, Osterbrock, Donald E., & Pogge, Richard W. 1987, ApJ, 323, 108 7. “The circumnuclear environment of the nearby non-interacting Seyfert galaxies NGC 5273 and NGC 3516”, Pogge, R. W., 1988, LNP, 307, 46 8. “An Extended Ionizing Radiation Cone from the Nucleus of the Seyfert 2 Galaxy NGC 1068”, Pogge, Richard W. 1988, ApJ, 328, 519 9. “Extended Ionized Gas in the Seyfert 2 Galaxy NGC 4388”, Pogge, Richard W. 1988, ApJ, 332, 702 10. “OTS 1809+314 and the Gamma-Ray Burst GB 790325b”, Hartmann, Dieter, Pogge, Richard W., Hurley, Kevin, Vrba, Frederick J., & Jennings, Mark C.
    [Show full text]