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The Agb Newsletter
THE AGB NEWSLETTER An electronic publication dedicated to Asymptotic Giant Branch stars and related phenomena Official publication of the IAU Working Group on Abundances in Red Giants No. 208 — 1 November 2014 http://www.astro.keele.ac.uk/AGBnews Editors: Jacco van Loon, Ambra Nanni and Albert Zijlstra Editorial Dear Colleagues, It is our pleasure to present you the 208th issue of the AGB Newsletter. The variety of topics is, as usual, enormous, though post-AGB phases feature prominently, as does R Scuti this time. Don’t miss the announcements of the Olivier Chesneau Prize, and of three workshops to keep you busy and entertained over the course of May–July next year. We look forward to receiving your reactions to this month’s Food for Thought (see below)! The next issue is planned to be distributed around the 1st of December. Editorially Yours, Jacco van Loon, Ambra Nanni and Albert Zijlstra Food for Thought This month’s thought-provoking statement is: What is your favourite AGB star, RSG, post-AGB object, post-RSG or PN? And why? Reactions to this statement or suggestions for next month’s statement can be e-mailed to [email protected] (please state whether you wish to remain anonymous) 1 Refereed Journal Papers Evolutionary status of the active star PZ Mon Yu.V. Pakhomov1, N.N. Chugai1, N.I. Bondar2, N.A. Gorynya1,3 and E.A. Semenko4 1Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya 48, 119017, Moscow, Russia 2Crimean Astrophysical Observatory, Nauchny, Crimea, 2984009, Russia 3Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetskij prospekt, 13, Moscow 119991, Russia 4Special Astrophysical Observatory of Russian Academy of Sciences, Russia We use original spectra and available photometric data to recover parameters of the stellar atmosphere of PZ Mon, formerly referred as an active red dwarf. -
Appendix: Spectroscopy of Variable Stars
Appendix: Spectroscopy of Variable Stars As amateur astronomers gain ever-increasing access to professional tools, the science of spectroscopy of variable stars is now within reach of the experienced variable star observer. In this section we shall examine the basic tools used to perform spectroscopy and how to use the data collected in ways that augment our understanding of variable stars. Naturally, this section cannot cover every aspect of this vast subject, and we will concentrate just on the basics of this field so that the observer can come to grips with it. It will be noticed by experienced observers that variable stars often alter their spectral characteristics as they vary in light output. Cepheid variable stars can change from G types to F types during their periods of oscillation, and young variables can change from A to B types or vice versa. Spec troscopy enables observers to monitor these changes if their instrumentation is sensitive enough. However, this is not an easy field of study. It requires patience and dedication and access to resources that most amateurs do not possess. Nevertheless, it is an emerging field, and should the reader wish to get involved with this type of observation know that there are some excellent guides to variable star spectroscopy via the BAA and the AAVSO. Some of the workshops run by Robin Leadbeater of the BAA Variable Star section and others such as Christian Buil are a very good introduction to the field. © Springer Nature Switzerland AG 2018 M. Griffiths, Observer’s Guide to Variable Stars, The Patrick Moore 291 Practical Astronomy Series, https://doi.org/10.1007/978-3-030-00904-5 292 Appendix: Spectroscopy of Variable Stars Spectra, Spectroscopes and Image Acquisition What are spectra, and how are they observed? The spectra we see from stars is the result of the complete output in visible light of the star (in simple terms). -
Further Observations of the Lambda 10830 He Line in Stars and Their Significance As a Measure of Stellar Activity
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) or I CALIFORNIA INSTITUTE OF TECHNOLOGY BIG BEAR SOLA R OBSERVATORY HALE OBSERVATORIES 4 I r -b cb c^ a y CNN (NASA-CR-145974) FURTHER CBSEPVATIONS CF N76-14992 THE LAMEDA 1083u He LING, IN STARS AND THEIR SIGNIFIC!NCE AS A MEAEURE OF STELLAR ACTIVITY (dale CbseEvatories, Pasadena, Unclas Calif.) 28 p HC $4.('. CSCL J3A G3;89 1,7726 t I FURTHER OBSERVATIONS OF THE XZ0830 HE LINE IN STARS AND THEIR SIGNIFICANCE AS A MEASURE OF STELLAR ACTIVITY H. Zirin HALE OBSERVATORIES CARNEGIE INSTITUTION OF WASHINGTON CALIFORNIA INSTITUTE OF TECHNOLOGY BBSO #0150 November, 1975 ABSTRACT Measurements of the x10830 He line in 198 stars are given, f along with data on other features in that spectral range. Nearly 80% of all G and K stars show some 110830; of these, half are variable and 1/4 show emission. -
VSSC 143Colour B.Pmd
British Astronomical Association VARIABLE STAR SECTION CIRCULAR No 143, March 2010 Contents RZ Cassiopeiae 2009 Phase Diagram ....................................... inside front cover From the Director ............................................................................................... 1 Eclipsing Binary News ...................................................................................... 2 KT Eridani (=Nova Eridani 2009) ...................................................................... 4 Mapping the Accretion Flows in Compact Binaries (VSS Meeting 2009) ...... 7 Some Stars I Don’t Observe .................................................................. 8 3C66A .............................................................................................................. 10 Recurrent Object Programme News ................................................................. 11 RU Herculis Light Curve .................................................................................. 14 First Acquaintance with AI Draconis ............................................................... 15 Long Term Polar Monitoring Programme - An Interim Report ........................ 18 IBVS 5911 - 5926 ............................................................................................. 23 Binocular Priority List ..................................................................................... 24 Eclipsing Binary Predictions ............................................................................ 25 Database for Amateur -
Resolving the Nature of RV Tauri Variable Systems Using Unprecedented Observations From
Stellar Evolution at the Crossroads: Resolving the Nature of RV Tauri Variable Systems Using Unprecedented Observations From the Kepler and XMM–Newton Space Telescopes By Laura Daniela Vega Dissertation Submitted to the Faculty of the Graduate School of Vanderbilt University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY in Astrophysics March 31, 2021 Nashville, Tennessee Approved: Keivan G. Stassun, Ph.D. Andreas A. Berlind, Ph.D. Patricia T. Boyd, Ph.D. J. Kelly Holley-Bockelmann, Ph.D. Rodolfo Montez Jr., Ph.D. Eric M. Schlegel, Ph.D. DEDICATION I dedicate this dissertation to all those who have inspired, encouraged, mentored, cared, and supported me on this journey to become an astrophysicist. ii ACKNOWLEDGMENTS This PhD could not have been possible on my own. I would like to take this moment to express my sincere thanks to all my family and friends who have cheered me on from the start. And to all the gentle people who have crossed my path, who I have either learned from or who have simply been kind to me at any point in this journey, thank you. Gabriel, thank you for your encouraging words and the countless moments you boosted my self-esteem when I did not believe in myself... Thank you for believing in me. Un agradecimiento especial a mama, daddy, Adriana, y Joel por su amor incondicional. Daddy (my Luna) and Mama (my Vega): gracias por llevarnos a Mexico´ a visitar familia cada verano desde que eramos´ pequenos.˜ Admirando el cielo repleto de estrellas durante nuestros viajes de noche en carretera, en el bello desierto montaoso Mexicano, fue una de mis inspiraciones para querer estudiar el universo. -
Smithsonian Miscellaneous Collections
SMITHSONIAN MISCELLANEOUS COLLECTIONS. 004 BIBLIOGRAPHY ASTKONOMY: FOR THE YEAR 1887 BY WILLIAM C. WINLOCK, ASSISTANT ASTRONOMER, UNITED STATES NAVAL OBSERVATORY. WASHINGTON: PUBLISHED BY THE SMITHSONIAN INSTITUTION. 1888. PRINTED AND STEREOTYPED BY JUDD & DETWEILER. AT WASHINGTON. D, 0. BIBLIOGRAPHY OF ASTRONOMY*. 1887. BY WILLIAM C. WINLOCK. I The following subject-index of astronomy for 1887 was originally compiled as an appendix to a general review of the progress of astronomy during that year, and though not exhaustive, it may, perhaps, be found a useful reference list. Important contributions to astronomy published during 1887 in scientific journals and trans- actions of societies, as well as all more elaborate publications that have come to the compiler's notice, have been included—a few titles being taken from reviews, or book- catalogues. Observations of asteroids and comets, except those of the comets of 1887, have generally been omitted. The prices quoted are usually from Friedlander's Naturae Novltates, in German "marks" (1 Mark = 100 Pfennige = 1 franc 25 centimes = 25 cents, nearly.) The abbreviated titles will probably be readily understood by those familiar with scientific periodicals without special explanation, beyond the following list of less obvious contractions. Abstr. — 4 BIBLIOGRAPHY OP ASTRONOMY: 1887. Aberration (Constant of) Continued. HouzEAU (J. C.) Note sur une mothode pour determiner la constante de I'aber- ration. 4 p. 8vo. Bruxelles, 1887. Bull, de I'acad. roy. de Belg., 3. s. 13, no. 2. Methode pour determiner la constante de I'aberration. Compt. Eend., 104: 278. Note additionelle sur la mesure de 1 "aberration. Ibid., 563. LoEWY (M.) Nouvelle methode pour la determination de la constante de I'aber- ration. -
First Detection of Surface Magnetic Fields in Post-AGB Stars: the Cases
Mon. Not. R. Astron. Soc. 000, 1–11 (2014) Printed 5 September 2021 (MN LATEX style file v2.2) First detection of surface magnetic fields in Post-AGB stars : the cases of U Monocerotis and R Scuti L. Sabin1;2?, G.A. Wade3 and A. Lebre` 4 1 Instituto de Astronom´ıa y Meteorolog´ıa, Departamento de F´ısica, CUCEI, Universidad de Guadalajara, Av. Vallarta 2602, C.P. 44130, Guadalajara, Jal., Mexico 2 Instituto de Estudios Avanzados de Baja California, A. C., Av. Obregon´ 1755, 22800 Ensenada, BC, Mexico. 3 Department of Physics, Royal Military College of Canada, PO Box 17000, Station Forces, Kingston, Ontario K7K 7B4, Canada. 4 Laboratoire Univers et Particules de Montpellier - CNRS and Universite´ Montpellier II - Place E. Bataillon, 34 090 Montpellier, France Accepted 2014 October 10. Received 2014 October 7; in original form 2014 September 11 ABSTRACT While several observational investigations have revealed the presence of magnetic fields in the circumstellar envelopes, jets and outflows of post-Asymptotic Giant Branch stars (PAGBs) and planetary nebulae (PNe), none has clearly demonstrated their presence at the stellar surface. The lack of information on the strength of the surface magnetic fields pre- vents us from performing any thorough assessment of their dynamic capability (i.e. material mixing, envelope shaping, etc). We present new high resolution spectropolarimetric (Stokes V ) observations of a sample of PAGB stars, realised with the instruments ESPaDOnS and Narval, where we searched for the presence of photospheric magnetic fields. Out of the seven targets investigated the RV Tauri stars U Mon and R Sct display a clear Zeeman signature and return a definite detection after performing a least squares deconvolution (LSD) analysis. -
The Stellar Heavens
M ed u m 8vo h e 1 05 . 6d . i . , clot xtra, F L A M M A R I O N ’S P O P U LA R A S T R O N O M Y Tr nslated m the e c . ELLA G E a fro Fr n h by J RD OR , With 3 Plates and 288 Ill ustrations . The six books into which the b ook is d ivid ed give a very lu cid and accu rate d esc ription of t he knowledge whi ch has be e n acquired of the m v b od e o f c e b h e ec he m and h c c i o ing i s spa . ot as r sp ts t ir otions p ysi al onst in e m of f t he a we can e e . N ot tu rions. O transl tion only sp ak t r s prais d e it e e e e the a b u t M r . e has dd ed u efu e only o s w ll r pr s nt origin l , Gor a s l not s f r t he u e of b t he f m u d e and has o p rpos ringing in or ation p to at , also — — increase d the nu mber already very consid e rable o f t he e xc e lle nt illustra t ha t he is l e bec m e ul in E d it has tions , so t work ik ly to o as pop ar nglan as ' — i F A tlzene u m . -
Meteor Csillagászati Évkönyv – 2017
ISSN 0866 - 2851 9 7 7 0 8 6 6 2 8 5 0 0 2 Ár: 3000 Ft meteor csillagászati évkönyv 2017 csillagászati évkönyv m e t e o 2017 r METEOR CSILLAGÁSZATI ÉVKÖNYV 2017 METEOR CSILLAGÁSZATI ÉVKÖNYV 2017 MCSE – 2016. OKTÓBER–NOVEMBER METEOR CSILLAGÁSZATI ÉVKÖNYV 2017 MCSE – 2016. OKTÓBER–NOVEMBER meteor csillagászati évkönyv 2017 Szerkesztette: Benkõ József Mizser Attila Magyar Csillagászati Egyesület www.mcse.hu Budapest, 2016 METEOR CSILLAGÁSZATI ÉVKÖNYV 2017 MCSE – 2016. OKTÓBER–NOVEMBER Az évkönyv kalendárium részének összeállításában közremûködött: Bagó Balázs Görgei Zoltán Kaposvári Zoltán Kernya János Gábor Kiss Áron Keve Kovács József Molnár Péter Sánta Gábor Sárneczky Krisztián Szabadi Péter Szabó M. Gyula Szabó Sándor Szôllôsi Attila A kalendárium csillagtérképei az Ursa Minor szoftverrel készültek. www.ursaminor.hu Szakmailag ellenôrizte: Szabados László A kiadvány a Magyar Tudományos Akadémia támogatásával készült. További támogatóink mindazok, akik az SZJA 1%-ával támogatják a Magyar Csillagászati Egyesületet. Adószámunk: 19009162-2-43 Felelôs kiadó: Mizser Attila Nyomdai elôkészítés: Kármán Stúdió, www.karman.hu Nyomtatás, kötészet: OOK-Press Kft., www.ookpress.hu Felelôs vezetô: Szathmáry Attila Terjedelem: 20,5 ív fekete-fehér + 12 oldal színes melléklet 2016. november ISSN 0866-2851 METEOR CSILLAGÁSZATI ÉVKÖNYV 2017 MCSE – 2016. OKTÓBER–NOVEMBER Tartalom Bevezetô ................................................... 7 Kalendárium ............................................... 13 Cikkek Kereszturi Ákos: Elsô eredmények a Plútó -
2015 CFHT Annual Report
2015 CFHT Annual Report Table of Contents Director’s Message…………………………………………………………………………………… 3 Science Report…………………………………………………........................................... 5 Maunakea Observatories and NASA Space Telescopes Find Galaxy ………. 5 Hot Jupiters Courting Baby Stars? ……………………….………………………………… 5 Faint Galaxies in the Virgo Cluster…………………………………………………………. 6 Mysterious, Massive, Magnetic Stars……………………………………….……………. 8 First Discovery of a Magnetic delta Scuti Star…......................................... 9 Engineering Report…………..………………………………….…………………………………… 10 SITELLE…….………………………………………………….……………………………………..….. 10 SPIRou ………………………………………………………………………………….…………….… 11 MegaCam ……………………………………….………………………………………………….… 12 GRACES….….…….………………………………………………………………………….…………. 14 Facilities Development……………………………….…………………….………………….… 15 MSE Report………………………………………………………………………………………………. 17 Administration Report….………………………………………………….………………………. 19 Overview…………..……………………………….…………………………………………………… 19 Summary of 2015 Finances….…….………………………………………………………….. 19 Building Renovations and Administration Activities……….………………………. 20 Staff Safety….……………………………………………………….………………………….……. 21 Arrivals and Departures…..…………………………………………………….………………. 22 Organization Chart ………………….………………………………………….….……………… 25 Staff List……………………………………………………………………………….………………… 26 Outreach Report……………………………………………………………………….………………. 27 2015 Publications…..………………………………………………………………….……………… 33 Front and back covers: The spiral galaxy Messier 98, as imaged by CFHT’s MegaCam, is shown on the front and back covers -
IUE References from 1978 Until June 2001
IUE REFERENCES from 1978 until June 2001 ¾ ½;4 J. Fernley ½ , P. Pitts , M. Barylak ¿ ¿ ¿ R. Gonzalez-Riestra´ ¿ ,E.Solano ,A.Talavera ,F.Rodr´ıguez ½ ESA IUE Observatory, PO Box 50727, 28080 Madrid, Spain ¾ NASA GSFC, Greenbelt, Maryland ¿ Laboratorio de Astrof´ısica Espacial y F´ısica Fundamental PO Box 50727, 28080 Madrid, Spain 4 Affiliated with the Astrophysics Division, Space Science Department ESTEC, the Netherlands We have compiled a list of references to IUE publications covering the period from 1978 until June 2001. This compilation is based upon earlier works of Mead et al. (1986), Pitts (1991) and our own. The IUE satellite has provided the scientific community with over 110,000 UV spectra which are now in the public domain. Prospective user of these IUE data are provided with a list that holds a total of 3776 IUE papers from the following journals: Journal Abbreviation Nr. Astronomical Journal AJ 200 Astronomy and Astrophysics A&A 982 Astronomy and Astrophysics Supplement A&AS 94 Astrophysical Journal APJ 1513 Astrophysical Journal Supplement APJS 112 Astrophysics and Space Science AP&SS 69 Advances in Space Research ASR 3 Geophysical Research Letters GRL 10 Irish Astronomical Journal IAJ 2 Icarus ICARUS 56 Journal of Geophysical Research JGR 19 Monthly Notices of the Royal Astr. Soc. MNRAS 410 Nature NATURE 53 Proceedings of the National Academy of Sience PNAS 2 Proceedings Astron. Soc. of Australia PASA 3 Publications Astron. Soc. of Japan PASJ 6 Publications of the Astron.Soc.of Pacific PASP 167 Revista Mexicana de Astronomia y Astrofisica RMAA 18 Science SCIENCE 2 Others (BAIC, M&P, RSPT, etc.) 55 Total 3776 We trust that this compilation is useful although we have not added other publications like meeting abstracts, conference proceedings, or other popular articles. -
Annual Report 2014-2015
AAVSO The American Association of Variable Star Observers Annual Report 2014–2015 Annual Report 2012 –2013 The American Association of Variable Star Observers AAVSO Annual Report 2014–2015 The American Association of Variable Star Observers 49 Bay State Road Cambridge, MA 02138-1203 USA Telephone: 617-354-0484 Fax: 617-354-0665 email: [email protected] website: https://www.aavso.org Annual Report Website: https://www.aavso.org/annual-report On the cover... Stella Kafka and Sara Beck leading a seminar at Girls Inc., Lynn, Massachusetts. Vina Hing and Linh Thuy Nguyen with their mentor Giorgio De Scala, Prairiewood High School, New South Wales, Australia. These students won first prize at SciCon15. Michael Cook, Andrew Pearce, Doug Welch, and Bill Goff at the Ball State University Observatory during the 2015 Spring Meeting. Picture credits In additon to images from the AAVSO and its archives, the editors gratefully acknowledge the following for their image contributions: Glenn Chaple, Michael Cook, Giorgio De Scala, Shawn Dvorak, Mary Glennon, Bill Goff, Barbara Harris,Carl Knight, Mario Motta, NASA, Gary Poyner, Msgr. Ronald Royer, the Mary Lea Shane Archives of the Lick Observatory, Chris Stephan, and Wheatley, et al. 2003, MNRAS, 345, 49. Thanks to Al Holm, Carol Beaman, Rebecca Turner, and Sara Beck for the meeting photos Table of Contents 1. About the AAVSO Vision and Mission Statement 1 About the AAVSO 1 What We Do 2 What Are Variable Stars? 3 Why Observe Variable Stars? 3 The AAVSO International Database 4 Observing Variable Stars 6 Services to Astronomy 7 Education and Outreach 9 2.