DOCSLIB.ORG

University of Hawai'i, Institute for Astronomy Publications in Calendar

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
University of Hawai'i, Institute for Astronomy Publications in Calendar University of Hawai‘i, Institute for Astronomy Publications in Calendar Year 2004 The names of authors listed as affiliated with IfA in each ar- &Wainscoat, R. J. Twenty-Three High-Redshift Super- ticle are in boldface. novae from the Institute for Astronomy Deep Survey: Doubling the Supernova Sample at z > 0.7. ApJ, 602, Abazajian, K., et al., including Siegmund, W. A., & Sza- 571–594 (2004) pudi, I. The Second Data Release of the Sloan Digital Sky Survey. AJ, 128, 502–512 (2004) Bendo, G. J., & Joseph, R. D. Nuclear Stellar Populations in the Infrared Space Observatory Atlas of Bright Spiral Abbas, M. M., LeClair, A., Owen, T., et al. The Nitrogen Galaxies. AJ, 127, 3338–3360 (2004) Isotopic Ratio in Jupiter’s Atmosphere from Observations by the Composite Infrared Spectrometer on the Cassini Bettoni, D., Mazzei, P., Della Valle, A., Franceschini, G. D. Spacecraft. ApJ, 602, 1063–1074 (2004) A., & Aussel, H. Optical and Spectroscopic Follow-Up of the Deeper FIR Selected Sample. Mem. Soc. Astron. Abel, N. P., Brogan, C. L., Ferland, G. J., O’Dell, C. R., Italiana Suppl., 5, 267–271 (2004) Shaw, G., & Troland, T. H. Physical Conditions in Orion’s Veil. ApJ, 609, 247–260 (2004) Beuzit, J.-L., et al., including Roddier, C., Roddier, F., & Mart´ın, E. L. New Neighbours. III. 21 New Compan- Allen, S. W., Schmidt, R. W., Ebeling, H., Fabian, A. C., ions to Nearby Dwarfs, Discovered with Adaptive Optics. &van Speybroeck, L. Constraints on Dark Energy from A&A, 425, 997–1008 (2004) Chandra Observations of the Largest Relaxed Galaxy Clusters. MNRAS, 353, 457–467 (2004) Binzel, R. P., Rivkin, A. S., Stuart, J. S., Harris, A. W., Bus, S. J., & Burbine, T. H. Observed Spectral Properties of Andersen, M., Knude, J., Reipurth, B., Castets, A., Nyman, Near-Earth Objects: Results for Population Distribution, L. A.,˚ McCaughrean, M. J., & Heathcote, S. Molecular Source Regions, and Space Weathering Processes. Icarus, Cloud Structure and Star Formation near HH 216 in M 16. 170, 259–294 (2004) A&A, 414, 969– 978 (2004) Boehnhardt, H., et al., including Meech, K. Results from the Andrews, S. M., Reipurth, B., Bally, J., & Heathcote, S. R. ESO Large Program on Transneptunian Objects and Cen- The Irradiated Herbig-Haro Jets Near σ Orionis. ApJ, taurs. Earth, Moon & Planets, 92, 145–156 (2003; c 606, 353–368 (2004) 2004) Andrews, S. M., Rothberg, B., & Simon, T. Mid- Boesgaard, A. M. The Light Elements: Lithium, Beryllium, Infrared and Submillimeter Observations of the Illumi- and Boron. In Carnegie Observatories Astrophys. Ser., nating Source of McNeil’s Variable Nebula. ApJ, 610, Vol. 4: Origin and Evolution of the Elements (Cambridge L45–L48 (2004) Univ. Press), 117–137 (2004) Ardila, D. R., et al., including Williams, J. P. AResolved Boesgaard, A. M., Armengaud, E., &King, J. R. Beryl- Debris Disk around the G2 V Star HD 107146. ApJ, 617, lium Abundances in F and G Dwarfs in Praesepe and L147–L150 (2004) Other Young Clusters from Keck HIRES Observations. Audard, M., et al., including Simon, T. Coronae of Cool ApJ, 605, 864–873 (2004) Stars. In IAU Symposium 219: Stars as Suns: Activity, Boesgaard, A. M., Armengaud, E., King, J. R., Deliyan- Evolution, and Planets, 243–248. nis, C. P., & Stephens, A. The Correlation of Lithium and 2 Avila, R., & Chun, M. R. AMethod for High-Resolution CN Beryllium in F and G Field and Cluster Dwarf Stars. ApJ, Profiling in the First Few Hundred Meters. Proc. SPIE, 613, 1202–1212 (2004) 5490, 742–748 (2004) Boesgaard, A. M., McGrath, E. J., Lambert, D. L., & Barger, A. J., ed. Supermassive Black Holes in the Dis- Cunha, K. Boron Benchmarks for the Galactic Disk. ApJ, tant Universe. Astrophys. & Space Sci. Library, Vol. 308 606, 306–318 (2004) (Kluwer, 2004) Bottinelli, S., & Williams, J. P. Modeling the Millimeter Barnes, J. E. Shock-induced Star Formation in a Model of Emission from the Cepheus A Young Stellar Cluster: Ev- the Mice. MNRAS, 350, 798–808 (2004) idence for Large Scale Collapse. A&A, 421, 1113–1119 Barris, B. J., & Tonry, J. L. Redshift-independent Distances (2004) to Type Ia Supernovae. ApJ, 613, L21–L24 (2004) Bottinelli, S., Ceccarelli, C., Lefloch, B., Williams, J. P., et Barris, B. J., Tonry, J. L., et al., including Aussel, H., al. Complex Molecules in the Hot Core of the Low-Mass Chambers, K. C., Connelley, M. S., Donovan, D., Protostar NGC 1333 IRAS 4A. ApJ, 615, 354–358 (2004) Henry, J. P., Kaiser, N., Liu, M. C., Mart´ın, E. L., 1 Bottinelli, S., Ceccarelli, C., Neri, R., Williams, J. P., et Burke, B. E., et al., including Tonry, J., Luppino, G., & al. Near-Arcsecond Resolution Observations of the Hot Onaka, P. The Orthogonal-Transfer Array: A New CCD Corino of the Solar-Type Protostar IRAS 16293-2422. Architecture for Astronomy. Proc. SPIE, 5499, 185–192 ApJ, 617, L69–L72 (2004) (2004) Bresolin, F., Garnett, D. R., & Kennicutt, R. C. Abundances Butler, N., et al., including Wainscoat, R., Ebeling, H., & of Metal-rich H II Regions in M51. ApJ, 615, 228–241 Luppino, G. Results of X-ray and Optical Followup Ob- (2004) servations of the Short/Hard GRB 020531. In ASP Conf. Bresolin, F., & Kudritzki, R. P. Stellar Winds of Hot Ser. 312: Third Rome Workshop on Gamma-Ray Bursts Massive Stars Nearby and Beyond the Local Group. In in the Afterglow Era, 201–204 Carnegie Observatories Astrophys. Ser., Vol. 4: Origin Capak, P. L. Probing Global Star and Galaxy Formation Us- and Evolution of the Elements (Cambridge Univ. Press), ing Deep Multi-Wavelength Surveys. PhD Thesis, UMI 283–296 (2004) Publ. No. 3139760 (2004) Bresolin, F., Pietrzynski,´ G., Gieren, W., Kudritzki, R., Capak, P., Cowie, L. L., Hu, E. M., Barger, A. J., et al. A Przybilla, N., &Fouque,´ P. On the Photometric Vari- Deep Wide-Field, Optical, and Near-Infrared Catalog of ability of Blue Supergiants in NGC 300 and Its Impact a Large Area around the Hubble Deep Field North. AJ, on the Flux-weighted Gravity-Luminosity Relationship. 127, 180–198 (2004) ApJ, 600, 182–187 (2004) Carr, J. S., Tokunaga, A. T., &Najita, J. Hot H2O Emission Briel, U. G., Finoguenov, A., & Henry, J. P. EPIC-XMM- and Evidence for Turbulence in the Disk of a Young Star. Newton Observations of Two Nearby Galaxy Clusters. ApJ, 603, 213–220 (2004) Proc. SPIE, 5488, 156–164 (2004) Carraro, G., Bresolin, F., Villanova, S., Matteucci, F., Patat, Briel, U. G., Finoguenov, A., & Henry, J. P. XMM-Newton F.,&Romaniello, M. Metal Abundances in Extremely EPIC Observation of the Galaxy Cluster A 3667. A&A, Distant Galactic Old Open Clusters. I. Berkeley 29 and 426, 1–9 (2004) Saurer 1. AJ, 128, 1676–1683 (2004) Brittain, S. D., Simon, T., Kulesa, C., & Rettig, T. W. Inter- Castets, A., Reipurth, B., &Loinard, L. Millimeter Observa- + α stellar H3 Line Absorption toward LkH 101. ApJ, 606, tions of the HH 222 Region. A&A, 427, 895–899 (2004) 911–916 (2004) Chiang, E. I., Millis, R. L., Buie, M. W., Wasserman, L. H. Brogan, C. L., Devine, K. E., Lazio, T. J., Kassim, N. E., & Meech, K. J. Resonant and Secular Families of the Tam, C. R., Brisken, W. F., Dyer, K. K., & Roberts, Kuiper Belt. Earth, Moon & Planets, 92, 49–62 (2003; M. S. E. A Low-Frequency Survey of the Galactic Plane c 2004) = ◦ Near l 11 :Discovery of Three New Supernova Rem- Chon, G., Challinor, A., Prunet, S., Hivon, E., & Szapudi, nants. AJ, 127, 355–367 (2004) I. Fast Estimation of Polarization Power Spectra Using Brogan, C. L., Goss, W. M., Lazendic, J. S., & Green, A. J. Correlation Functions. MNRAS, 350, 914–926 (2004) OH (1720 MHz) Maser Search toward the Large Magel- Clark, B. E., Bus, S. J., Rivkin, A. S., Shepard, M. K., lanic Cloud. AJ, 128, 700–708 (2004) &Shah, S. Spectroscopy of X-Type Asteroids. AJ, 128, Budavari,´ T., Connolly, A. J., Szalay, A. S., Szapudi, I., 3070–3081 (2004) Csabai, I., & Scranton, R. Angular Clustering with Pho- Clarke, C., Reipurth, B., &Delgado-Donate, E. Multiple tometric Redshifts. In Astrophys. & Space Sci. Library, Protostars, Jets, and the Origin of Brown Dwarfs. In Vol. 301: Multiwavelength Cosmology (Kluwer), 55–58 IAU Colloquium 191: The Environment and Evolution (2004) of Double and Multiple Stars, Rev. Mexicana Astron. As- Buie, M. W., et al., including Meech, K..Procedures, Re- trof´ıs. Conf. Ser. 21, 184–194 (2004) sources and Selected Results of the Deep Ecliptic Survey. Coil, A. L., Newman, J. A., Kaiser, N., Davis, M., Ma, C., Earth, Moon & Planets, 92, 113–124 (2003; c 2004) Kocevski,D.D.,&Koo, D. C. Evolution and Color De- Buratti, B. J., et al., including Meier, R., & Owen, T. C. 9969 pendence of the Galaxy Angular Correlation Function: Braille: Deep Space 1 Infrared Spectroscopy, Geometric 350,000 Galaxies in 5 Square Degrees. ApJ, 617, 765– Albedo, and Classification. Icarus, 167, 129–135 (2004) 781 (2004) Burgett, W. S., et al. Substructure Analysis of Selected Low- Coil, A. L., et al., including Kaiser, N. The DEEP2 Galaxy Richness 2dFGRS Clusters of Galaxies. MNRAS, 352, Redshift Survey: Clustering of Galaxies in Early Data. 605–654 (2004) ApJ, 609, 525–538 (2004) Burke, B. E., et al., including Luppino, G. A., & Tonry, Comeron,´ F., Reipurth, B., Henry, A., & Fernandez,´ M. J. L. Broadband (200–1000 nm) Back-Illuminated CCD Extending the Census at the Bottom of the Stellar Mass Imagers. In Astrophys. & Space Sci. Library, Vol. 300: Function in Chamaeleon I. A&A, 417, 583–596 (2004) ScientificDetectors for Astronomy: The Beginning of a Cotˆ e,´ P., et al., including Tonry, J.
Load more

Recommended publications
  • FY08 Technical Papers by GSMTPO Staff
    AURA/NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation July 23, 2008 Revised as Complete and Submitted December 23, 2008 NGC 660, ~13 Mpc from the Earth, is a peculiar, polar ring galaxy that resulted from two galaxies colliding. It consists of a nearly edge-on disk and a strongly warped outer disk. Image Credit: T.A. Rector/University of Alaska, Anchorage NATIONAL OPTICAL ASTRONOMY OBSERVATORY NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation December 23, 2008 TABLE OF CONTENTS EXECUTIVE SUMMARY ............................................................................................................................. 1 1 SCIENTIFIC ACTIVITIES AND FINDINGS ..................................................................................... 2 1.1 Cerro Tololo Inter-American Observatory...................................................................................... 2 The Once and Future Supernova η Carinae...................................................................................................... 2 A Stellar Merger and a Missing White Dwarf.................................................................................................. 3 Imaging the COSMOS...................................................................................................................................... 3 The Hubble Constant from a Gravitational Lens.............................................................................................. 4 A New Dwarf Nova in the Period Gap............................................................................................................
    [Show full text]
  • TESTING MODELS of LOW-EXCITATION PHOTODISSOCIATION REGIONS with FAR-INFRARED OBSERVATIONS of REFLECTION NEBULAE Rolaine C
    The Astrophysical Journal, 578:885–896, 2002 October 20 # 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A. TESTING MODELS OF LOW-EXCITATION PHOTODISSOCIATION REGIONS WITH FAR-INFRARED OBSERVATIONS OF REFLECTION NEBULAE Rolaine C. Young Owl Department of Physics and Astronomy, University of California at Los Angeles, Mail Code 156205, Los Angeles, CA 90095-1562 Margaret M. Meixner1 and David Fong Department of Astronomy, University of Illinois, Urbana, IL 61801; [email protected], [email protected] Michael R. Haas NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035-1000; [email protected] Alexander L. Rudolph1 Department of Physics, Harvey Mudd College, 301 East 12th Street, Claremont, CA 91711; [email protected] and A. G. G. M. Tielens Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, Netherlands; [email protected] Received 2001 August 2; accepted 2002 June 24 ABSTRACT This paper presents Kuiper Airborne Observatory observations of the photodissociation regions (PDRs) in nine reflection nebulae. These observations include the far-infrared atomic fine-structure lines of [O i]63 and 145 lm, [C ii] 158 lm, and [Si ii]35lm and the adjacent far-infrared continuum to these lines. Our analysis of these far-infrared observations provides estimates of the physical conditions in each reflection nebula. In our sample of reflection nebulae, the stellar effective temperatures are 10,000–30,000 K, the gas densities are 4 Â 102 2 Â 104 cmÀ3, the gas temperatures are 200–690 K, and the incident far-ultraviolet intensities are 300–8100 times the ambient interstellar radiation field strength (1:2 Â 10À4 ergs cmÀ2 sÀ1 srÀ1).
    [Show full text]
  • Prof. Mustafa Türker ÖZKAN
    Prof. Mustafa Türker ÖZKAN OPfefricseo Pnhaol nIen:f +or9m0 2a1t2io 4n40 0369 Extension: 10294 EFmaxa iPl:h oznkea:n +t@9i0s t2a1n2b u4l4.e0d u0.3tr70 AWdedbr:e hstst:p :A/s/tarvoenso.imstia vneb uUlz.eadyu B.tirli/molzekrai nBtö/lümü, İstanbul Üniversitesi Beyazıt Yerleşkesi, 34119, Fatih-İstanbul EDodcutocraatteio, İnst aInnbfuol rÜmniavetriosintesi, Faculty of Science, Astronomi Ve Uzay Bilimleri, Turkey 1981 - 1987 UPonsdtegrrgardaudautaet, eİs, tİastnabnublu Ül nÜinveivresritseitsei,s Fi, aFcauclutylt oy fo Sfc Siecniecnec, eA, sAtrsotrnoonmomi Vi eV Ue zUazya By iBlimilimlerlei,r Ti, uTrukrekye 1y 917987 3- 1- 9189077 FEnogrliesihg, nB2 L Uapnpgeru Iangteersmediate Dissertations ADsotcrtoonroamtey, G aünnde Sşp Laeckee Slecrieinndceks,i 1D9o8ğ7u-Batı Asimetrisinin Nedenleri Üzerine, Istanbul University, Faculty of Science, APostsrtognraodmuya taen, dP lSapnaect ev eS cÇieifnt-cYeısld, 1ız9 Y8ö0rüngelerinde Büyük Eksen Dönmesi, Istanbul University, Faculty of Science, Research Areas aPnhdy sOicbss, eArsvtartoionnosm, yS taanrsd, ANsattruorpahl ySsciicesn, cSeusn and Solar Systems, Astronomy and Astrophysics: Instrumentation Techniques Academic Titles / Tasks APrsosofecsiastoer ,P Irsotafensbsuolr U, Insitvaenrbsuitly U, Fnaivceurltsyit yo,f FSaccieunltcye o, Af sStcrioencoem, Ay satnrodn Sopmacye a Sncdie Snpcaecse, 1S9c9ie5n c- eCso, n1t9in9u0e -s 1995 RAessiesatarcnht PArsosfisetsasnotr, ,İ Issttaannbbuul lÜ Unniviveerrssititeys,i ,F Faaccuultlyty o of fS Sccieiennccee, ,A Asstrtroonnoommyy a anndd S Sppaaccee S Sccieienncceess,
    [Show full text]
  • List of Poster Papers
    List of poster papers Downloaded from https://www.cambridge.org/core. IP address: 170.106.202.8, on 29 Sep 2021 at 04:56:15, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900083601 LIST OF POSTER PAPERS Ρ 1: Christian Doppler (1803- 1853): an Austrian scientist M. Firneis Ρ 2: Austrian astronomy today: a research initiative in stellar astrophysics M. Breger, E. A. Dorß, J. Hron, K. G. Strassmeier, W. W. Weiss, if. Oberhummer, A. Hanslmeier, G. Lustig, if. J. Schober Ρ 3: The Kuffner public observatory in Vienna P. Habison, E. Krebs Ρ 4: Inclination dependence of the mean spectral line shapes of RS CVn stars as evidence for polar spots A. P. Hatzes, S. S. Vbgt, T. F. Ramseyer, A. MiscA Ρ 5: Maximum Entropy spot mapping with simultaneous geometrical and orbital parameter fitting for contact binaries P. D. Hendry Ρ 6: Doppler imaging by the Mean Information Principle S. V. Berdyugina Ρ 7: Prospects of stellar tomographic imaging S. Jsinkov Ρ 8: A new tool for measuring stellar magnetic fields J. Babei, D. Queloz, P. North, M. Mayor Ρ 9: Fourier analysis of time-variable line profiles as a tool to evaluate latitudinal differential rotation A. F. Lanza, M. Rodonö Ρ 10: The interpretation of two-dimensional Fourier analysis of line-profile series Jinxin Hao Ρ 11: On the stability of starspot modelling. I. Zs. Kövari Ρ 12: On the stability of starspot modelling. II. Counteractions between spot parameter determination and inclination Zs.
    [Show full text]
  • A Photometric Study of Be Stars Located in the Seismology fields of COROT
    A&A 476, 927–933 (2007) Astronomy DOI: 10.1051/0004-6361:20078252 & c ESO 2007 Astrophysics A photometric study of Be stars located in the seismology fields of COROT J. Gutiérrez-Soto1,2,J.Fabregat1,2,J.Suso3, M. Lanzara3, R. Garrido4, A.-M. Hubert2, and M. Floquet2 1 Observatorio Astronómico, Universidad de Valencia, edificio Institutos de Investigación, polígono la Coma, 46980 Paterna, Valencia, Spain e-mail: [email protected] 2 GEPI, Observatoire de Paris, CNRS, Université Paris Diderot; place Jules Janssen 92195 Meudon Cedex, France 3 GACE-ICMUV, edificio Institutos de Investigación, polígono la Coma, 46980 Paterna, Valencia, Spain 4 Instituto de Astrofísica de Andalucía (CSIC), calle Camino Bajo de Huétor, 24. 18008, Granada, Spain Received 10 July 2007 / Accepted 28 September 2007 ABSTRACT Context. In preparation for the COROT mission, an exhaustive photometric study of Be stars located in the seismology fields of the mission has been performed. The very precise and long-time-spanned photometric observations gathered by the COROT satellite will give important clues on the origin of the Be phenomenon. Aims. The aim of this work is to find short-period variable Be stars located in the seismology fields of COROT, and to study and characterise their pulsational properties. Methods. Light curves obtained at the Observatorio de Sierra Nevada, together with data from Hipparcos and ASAS-3 for a total of 84 Be stars, were analysed in order to search for short-term variations. We applied standard Fourier techniques and non-linear least-square fitting to the time series. Results. We found 7 multiperiodic, 21 mono-periodic and 26 non-variable Be stars.
    [Show full text]
  • Information Bulletin on Variable Stars
    COMMISSIONS AND OF THE I A U INFORMATION BULLETIN ON VARIABLE STARS Nos November July EDITORS L SZABADOS K OLAH TECHNICAL EDITOR A HOLL TYPESETTING K ORI ADMINISTRATION Zs KOVARI EDITORIAL BOARD L A BALONA M BREGER E BUDDING M deGROOT E GUINAN D S HALL P HARMANEC M JERZYKIEWICZ K C LEUNG M RODONO N N SAMUS J SMAK C STERKEN Chair H BUDAPEST XI I Box HUNGARY URL httpwwwkonkolyhuIBVSIBVShtml HU ISSN COPYRIGHT NOTICE IBVS is published on b ehalf of the th and nd Commissions of the IAU by the Konkoly Observatory Budap est Hungary Individual issues could b e downloaded for scientic and educational purp oses free of charge Bibliographic information of the recent issues could b e entered to indexing sys tems No IBVS issues may b e stored in a public retrieval system in any form or by any means electronic or otherwise without the prior written p ermission of the publishers Prior written p ermission of the publishers is required for entering IBVS issues to an electronic indexing or bibliographic system to o CONTENTS C STERKEN A JONES B VOS I ZEGELAAR AM van GENDEREN M de GROOT On the Cyclicity of the S Dor Phases in AG Carinae ::::::::::::::::::::::::::::::::::::::::::::::::::: : J BOROVICKA L SAROUNOVA The Period and Lightcurve of NSV ::::::::::::::::::::::::::::::::::::::::::::::::::: :::::::::::::: W LILLER AF JONES A New Very Long Period Variable Star in Norma ::::::::::::::::::::::::::::::::::::::::::::::::::: :::::::::::::::: EA KARITSKAYA VP GORANSKIJ Unusual Fading of V Cygni Cyg X in Early November :::::::::::::::::::::::::::::::::::::::
    [Show full text]
  • A Tail Structure Associated with Protoplanetary Disk Around SU
    Draft version February 28, 2019 A Preprint typeset using LTEX style emulateapj v. 12/16/11 A TAIL STRUCTURE ASSOCIATED WITH PROTOPLANETARY DISK AROUND SU AURIGAE EIJI AKIYAMA1, EDUARD I. VOROBYOV2,3, HAUYU BAOBABU LIU4,5, RUOBING DONG5,6, JEROME de LEON7, SHENG-YUAN LIU5, MOTOHIDE TAMURA7,8,9 1Institute for the Advancement of Higher Education, Hokkaido University, Kita17, Nishi8, Kita-ku, Sapporo, 060-0817, Japan; [email protected] 2Department of Astrophysics, University of Vienna, Vienna 1018, Austria 3Research Institute of Physics, Southern Federal University, Rostov-on-Don, 344090, Russia 4European Southern Observatory, Karl Schwarzschild Str 2, 85748 Garching bei M¨unchen, Germany 5Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei, 10617, Taiwan 6Department of Astronomy/Steward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA 7Department of Astronomy, The University of Tokyo, 7-3-1, Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan 8Astrobiology Center of NINS, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588, Japan 9National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588, Japan Draft version February 28, 2019 ABSTRACT We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO (J=2– 1) line emission from the protoplanetary disk around T-Tauri star SU Aurigae (hereafter SU Aur). Previous observations in optical and near infrared wavelengths find a unique structure in SU Aur. One of the highlights of the observational results is that an extended tail-like structure is associated with the disk, indicating mass transfer from or into the disk.
    [Show full text]
  • Astrophysical Studies of Extrasolar Planetary Systems Using Infrared Interferometric Techniques Olivier Absil
    Astrophysical studies of extrasolar planetary systems using infrared interferometric techniques Olivier Absil To cite this version: Olivier Absil. Astrophysical studies of extrasolar planetary systems using infrared interferometric techniques. Astrophysics [astro-ph]. Université de Liège, 2006. English. tel-00124720 HAL Id: tel-00124720 https://tel.archives-ouvertes.fr/tel-00124720 Submitted on 15 Jan 2007 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Facult´edes Sciences D´epartement d’Astrophysique, G´eophysique et Oc´eanographie Astrophysical studies of extrasolar planetary systems using infrared interferometric techniques THESE` pr´esent´eepour l’obtention du diplˆomede Docteur en Sciences par Olivier Absil Soutenue publiquement le 17 mars 2006 devant le Jury compos´ede : Pr´esident: Pr. Jean-Pierre Swings Directeur de th`ese: Pr. Jean Surdej Examinateurs : Dr. Vincent Coude´ du Foresto Dr. Philippe Gondoin Pr. Jacques Henrard Pr. Claude Jamar Dr. Fabien Malbet Institut d’Astrophysique et de G´eophysique de Li`ege Mis en page avec la classe thloria. i Acknowledgments First and foremost, I want to express my deepest gratitude to my advisor, Professor Jean Surdej. I am forever indebted to him for striking my interest in interferometry back in my undergraduate student years; for introducing me to the world of scientific research and fostering so many international collaborations; for helping me put this work in perspective when I needed it most; and for guiding my steps, from the supervision of diploma thesis to the conclusion of my PhD studies.
    [Show full text]
  • Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
    Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis,
    [Show full text]
  • Stars Chien-De Lee (李建德)1, Wen-Ping Chen (陳文屏)1, 2, and Sheng-Yuan Liu (呂聖元)3
    A&A 592, A130 (2016) Astronomy DOI: 10.1051/0004-6361/201628332 & c ESO 2016 Astrophysics Evolutionary status of isolated B[e] stars Chien-De Lee (Nú·)1, Wen-Ping Chen (s文O)1; 2, and Sheng-Yuan Liu (BVC)3 1 Graduate Institute of Astronomy, National Central University, 300 Jhongda Road, 32001 Jhongli, Taiwan e-mail: [email protected] 2 Department of Physics, National Central University, 300 Jhongda Road, 32001 Jhongli, Taiwan 3 Institute of Astronomy and Astrophysics, Academia Sinica, 10617 Taipei, Taiwan Received 18 February 2016 / Accepted 18 May 2016 ABSTRACT Aims. We study a sample of eight B[e] stars with uncertain evolutionary status to shed light on the origin of their circumstellar dust. Methods. We performed a diagnostic analysis on the spectral energy distribution beyond infrared wavelengths, and conducted a census of neighboring region of each target to ascertain its evolutionary status. Results. In comparison to pre-main sequence Herbig stars, these B[e] stars show equally substantial excess emission in the near- infrared, indicative of existence of warm dust, but much reduced excess at longer wavelengths, so the dusty envelopes should be compact in size. Isolation from star-forming regions excludes the possibility of their pre-main sequence status. Six of our targets, including HD 50138, HD 45677, CD−24 5721, CD−49 3441, MWC 623, and HD 85567, have been previously considered as FS CMa stars, whereas HD 181615/6 and HD 98922 are added to the sample by this work. We argue that the circumstellar grains of these isolated B[e] stars, already evolved beyond the pre-main sequence phase, should be formed in situ.
    [Show full text]
  • Thesisthesis We Analyzed a Large Sample of Young Stars,, Coveringcovering Aa Massmass Rangerange of ~2 to ~20 Solar Masses
    UvA-DARE (Digital Academic Repository) Dusty disks around young stars Verhoeff, A. Publication date 2009 Document Version Final published version Link to publication Citation for published version (APA): Verhoeff, A. (2009). Dusty disks around young stars. General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:06 Oct 2021 Dusty Disks around Dusty Disks around Stars are formed through the collapse of giant molecular clouds.. During this contraction the matter spins up and naturally forms a circumstellar disk.. OnceOnce accretionaccretion comescomes toto aa halt,halt, thesethese disksdisks arare relatively stable.. SomeSome disksdisks areare kknown to last up to 10 Myrs.. MostMost disks however,, dissipatedissipate onon shorshorter time scales under the inuence of photoevaporation and planet formation. These disks,, consistingconsisting of 99% gas and 1% dust, have revealed a high variety of dust composition and geometry.
    [Show full text]
  • Download This Issue (Pdf)
    Volume 46 Number 2 JAAVSO 2018 The Journal of the American Association of Variable Star Observers Unmanned Aerial Systems for Variable Star Astronomical Observations The NASA Altair UAV in flight. Also in this issue... • A Study of Pulsation and Fadings in some R CrB Stars • Photometry and Light Curve Modeling of HO Psc and V535 Peg • Singular Spectrum Analysis: S Per and RZ Cas • New Observations, Period and Classification of V552 Cas • Photometry of Fifteen New Variable Sources Discovered by IMSNG Complete table of contents inside... The American Association of Variable Star Observers 49 Bay State Road, Cambridge, MA 02138, USA The Journal of the American Association of Variable Star Observers Editor John R. Percy Laszlo L. Kiss Ulisse Munari Dunlap Institute of Astronomy Konkoly Observatory INAF/Astronomical Observatory and Astrophysics Budapest, Hungary of Padua and University of Toronto Asiago, Italy Toronto, Ontario, Canada Katrien Kolenberg Universities of Antwerp Karen Pollard Associate Editor and of Leuven, Belgium Director, Mt. John Observatory Elizabeth O. Waagen and Harvard-Smithsonian Center University of Canterbury for Astrophysics Christchurch, New Zealand Production Editor Cambridge, Massachusetts Michael Saladyga Nikolaus Vogt Kristine Larsen Universidad de Valparaiso Department of Geological Sciences, Valparaiso, Chile Editorial Board Central Connecticut State Geoffrey C. Clayton University, Louisiana State University New Britain, Connecticut Baton Rouge, Louisiana Vanessa McBride Kosmas Gazeas IAU Office of Astronomy for University of Athens Development; South African Athens, Greece Astronomical Observatory; and University of Cape Town, South Africa The Council of the American Association of Variable Star Observers 2017–2018 Director Stella Kafka President Kristine Larsen Past President Jennifer L.
    [Show full text]