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145, September 2010
British Astronomical Association VARIABLE STAR SECTION CIRCULAR No 145, September 2010 Contents EG Andromedae Light Curve ................................................... inside front cover From the Director ............................................................................................... 1 Letter Page. Visual Observing ............................................................................ 4 Epsilon Aurigae Spectroscopically at Mid Eclipse .......................................... 5 Eclipsing Binary News ...................................................................................... 7 AO Cassiopeiae Phase Diagram ............................................................ 9 PV Cephei and Gyulbudaghian’s Nebula ........................................................ 10 WR140 Periastron Campaign Update .............................................................. 12 VSS Meeting, Pendrell Hall. The Central Stars of Planetary Nebulae ............ 14 RR Coronae Borealis 1993-2004 ...................................................................... 16 TU Cassiopeiae Phase Diagram 2005-2010 ..................................................... 18 Binocular Priority List ..................................................................................... 19 Eclipsing Binary Predictions ............................................................................ 20 Charges for Section Publications .............................................. inside back cover Guidelines for Contributing to the Circular ............................. -
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............................................................................................................ -
Stellar Evolution in Real Time: Models Consistent with Direct Observation of Thermal Pulse in T Ursae Minoris Laszl´ O´ Molnar´ ,1, 2 Meridith Joyce,3 Andl Aszl´ O´ L
Draft version June 6, 2019 Typeset using LATEX twocolumn style in AASTeX62 Stellar Evolution in Real Time: Models Consistent with Direct Observation of Thermal Pulse in T Ursae Minoris Laszl´ o´ Molnar´ ,1, 2 Meridith Joyce,3 andL aszl´ o´ L. Kiss1, 4 1Konkoly Observatory, MTA CSFK, Budapest, Konkoly Thege Mikl´os´ut15-17, Hungary 2MTA CSFK Lend¨uletNear-Field Cosmology Research Group, 1121, Budapest, Konkoly Thege Mikl´os´ut15-17, Hungary 3Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia 4Sydney Institute for Astronomy, School of Physics A29, University of Sydney, NSW 2006, Australia ABSTRACT Most aspects of stellar evolution proceed far too slowly to be directly observable in a single star on human timescales. The thermally pulsing asymptotic giant branch is one exception. The combination of state-of-the-art modelling techniques with data assimilated from observations collected by amateur astronomers over many decades provide, for the first time, the opportunity to identify a star occupying precisely this evolutionary stage. In this study, we show that the rapid pulsation period change and associated reduction in radius in the bright, northern variable star T Ursae Minoris are caused by the recent onset of a thermal pulse. We demonstrate that T UMi transitioned into a double-mode pulsation state, and we exploit its asteroseismic features to constrain its fundamental stellar parameters. We use evolutionary models from MESA and linear pulsation models from GYRE to track simultaneously the structural and oscillatory evolution of models with varying mass. We apply a sophisticated iterative sampling scheme to achieve time resolution ≤ 10 years at the onset of the relevant thermal pulses. -
Arxiv:2001.10147V1
Magnetic fields in isolated and interacting white dwarfs Lilia Ferrario1 and Dayal Wickramasinghe2 Mathematical Sciences Institute, The Australian National University, Canberra, ACT 2601, Australia Adela Kawka3 International Centre for Radio Astronomy Research, Curtin University, Perth, WA 6102, Australia Abstract The magnetic white dwarfs (MWDs) are found either isolated or in inter- acting binaries. The isolated MWDs divide into two groups: a high field group (105 − 109 G) comprising some 13 ± 4% of all white dwarfs (WDs), and a low field group (B < 105 G) whose incidence is currently under investigation. The situation may be similar in magnetic binaries because the bright accretion discs in low field systems hide the photosphere of their WDs thus preventing the study of their magnetic fields’ strength and structure. Considerable research has been devoted to the vexed question on the origin of magnetic fields. One hypothesis is that WD magnetic fields are of fossil origin, that is, their progenitors are the magnetic main-sequence Ap/Bp stars and magnetic flux is conserved during their evolution. The other hypothesis is that magnetic fields arise from binary interaction, through differential rotation, during common envelope evolution. If the two stars merge the end product is a single high-field MWD. If close binaries survive and the primary develops a strong field, they may later evolve into the arXiv:2001.10147v1 [astro-ph.SR] 28 Jan 2020 magnetic cataclysmic variables (MCVs). The recently discovered population of hot, carbon-rich WDs exhibiting an incidence of magnetism of up to about 70% and a variability from a few minutes to a couple of days may support the [email protected] [email protected] [email protected] Preprint submitted to Journal of LATEX Templates January 29, 2020 merging binary hypothesis. -
Pennsylvania Science Olympiad State Finals 2017 Astronomy C Division
PENNSYLVANIA SCIENCE OLYMPIAD STATE FINALS 2017 ASTRONOMY C DIVISION EXAM APRIL 29, 2017 TEAM NUMBER _____________ SCHOOL NAME_____________________________________ PARTICIPANTS__________________________________________________________________ _______________________________________________________________________________ INSTRUCTIONS: 1. Turn in all exam materials at the end of this event. Missing exam materials will result in immediate disqualification of the team in question. There is an exam packet, an image packet, and 3 blank answer sheets. 2. You may separate the exam pages. 3. Only the answers provided on the answer page will be considered. Do not write outside the designated spaces for each answer. You may write in the exam booklet. 4. Write your team number, school name, and participants’ names on the title page of the test booklet. By writing your participants’ names, you agree to the General Rules, Code of Ethics, and Spirit of the Problem as defined on the Science Olympiad website: https://www.soinc.org/code-ethics-general-rules. 5. Write your team number, school name, and participants’ names in the appropriate spaces on the answer sheets. 6. Each question is worth one point. Tiebreaker questions are indicated with a (T#) in which the number indicates the order of consultation in the event of a tie. Tiebreaker questions count toward the overall raw score, and are only used as tiebreakers when there is a tie. In such cases, (T1) will be examined first, then (T2), and so on until the tie is broken. There are 16 tiebreakers. 7. Pay close attention to the units given in the problem and the units asked for in the answer. 8. When the time is up, the time is up. -
COMMISSION G4 PULSATING STARS 1. Introduction 2. Notable
Transactions IAU, Volume XXXIA Reports on Astronomy 2018-2021 © 2021 International Astronomical Union Maria Teresa Lago, ed. DOI: 00.0000/X000000000000000X COMMISSION G4 PULSATING STARS PRESIDENT Jaymie Matthews VICE-PRESIDENT Robert Szabo ACTING PRESIDENT Robert Szabo ORGANIZING COMMITTEE Victoria Antoci, Hiromoto Shibahashi, Joyce Ann Guzik, Daniel Huber, Jadwiga Daszynska-Daszkiewicz TRIENNIAL REPORT 2018-2021 1. Introduction We are witnessing a renaissance of pulsating stars. These objects are cornerstones of stellar astrophysics { asteroseismology, galactic archaeology, and extragalactic science, as well. The renewed interest in pulsations and oscillations are boosted by the fact that more precise observations are being gathered than ever, more stars are monitored than ever before, and more continuous data sets are available than a mere few years ago. Both hardware (information technology and computing power) and software (machine learning and artificial intelligence) developments make it easier to cope with and analyze the large data sets (and models!), and synergies with Solar System studies and exoplanet hunting manifest in large surveys particularly useful for studying pulsations and oscillations. The European Space Agency's Gaia mission brought a revolution in stellar astrophysics in general, and in the astrophysics of pulsating and oscillating stars in particular. Homoge- neous and high-precision astrometric, photometric, and some low-resolution spectroscopic data are now available across all the sky, as well as across galactic -
Dr Meridith P. Joyce Research Interests Academic Work Experience Education Publications: First Authorships and Co-Leads Publicat
Dr Meridith P. Joyce [email protected] • +61.476.680.932 • W35 Mt Stromlo Observatory, Weston Creek, ACT 2611, Australia www.meridithjoyce.com • https://github.com/mjoyceGR • ADS Library: DrMeridithJoyce Research Interests Theoretical and computational astrophysics: stellar structure and evolution, precision stellar modeling across the mass spectrum, asteroseismology, stellar interiors, convection and mixing, numerical methods, astronomy software development. Optical astronomy: variable and oscillating stars, low-metallicity stars, globular clusters. Academic Work Experience RSAA Postdoctoral Fellow | Australian National University, September 2018{present South African Astronomical Observatory | Postgraduate research assistant, June 2017{November 2017 Massachusetts Institute of Technology | Research assistant, June{August 2015 Dartmouth College | Research assistant, September 2013{July 2018 Positions Held Concurrently ARC Centre of Excellence ASTRO3D | Associate investigator, November 2019{present Modules for Experiments in Stellar Astrophysics (MESA) developer, September 2019{present Konkoly Observatory | Visiting resident astronomer, periodic from January 2018{present University of Cape Town | Visiting academic, periodic from June 2017{January 2019 Education Ph.D. Physics and Astronomy | Dartmouth College, 2015{2018 | Prof. Brian Chaboyer, adviser On the Scope and Fidelity of 1-D Stellar Evolution Models M.S. Physics | Dartmouth College, 2013{2015 | Prof. Brian Chaboyer, adviser Investigating the Consistency of Stellar Evolution Models with Globular Cluster Observations via the Red Giant Branch Bump B.Sc. Mathematics, B.Sc. Physics | Bucknell University, 2009{2013 Publications: First authorships and co-leads 1. Meridith Joyce, Shing-Chi Leung, L´aszl´oMoln´ar,Michael J. Ireland, Chiaki Kobayashi, Ken'ichi Nomoto, Standing on the shoulders of giants: New mass and distance estimates for Betelgeuse through combined evolutionary, asteroseismic, and hydrodynamical simulations with MESA, ApJ, October 2020 2. -
JAAVSO 2008 the Journal of the American Association of Variable Star Observers
Volume 36 Number 1 JAAVSO 2008 The Journal of the American Association of Variable Star Observers Detection of the First Observed Outburst of DW Cancri Photometric light curve from all AAVSO V filter observations of DW Cnc between 2006 December 24 and 2007 February 04. Also in this issue... • Discovery and Observations of the Optical Afterglow of GRB 071010B • On the Connection Between CWA and RVA Stars • Studying Variable Stars Discovered Through Exoplanet-Transit Surveys 49 Bay State Road Cambridge, MA 02138 Complete table of contents inside... U. S. A. The Journal of the American Association of Variable Star Observers Editor Associate Editor Charles A. Whitney Elizabeth O. Waagen Harvard-Smithsonian Center for Astrophysics Assistant Editor 60 Garden Street Matthew Templeton Cambridge, MA 02138 Production Editor Michael Saladyga Editorial Board Priscilla J. Benson John R. Percy Wellesley College University of Toronto Wellesley, Massachusetts Toronto, Ontario, Canada Douglas S. Hall David B. Williams Vanderbilt University Indianapolis, Indiana Nashville, Tennessee Thomas R. Williams Houston, Texas The Council of the American Association of Variable Star Observers 2007–2008 Director Arne A. Henden President Paula Szkody Past President David B. Williams 1st Vice President Jaime Ruben Garcia 2nd Vice President Michael A. Simonsen Secretary Gary Walker Treasurer David A. Hurdis Clerk Arne A. Henden Councilors Barry B. Beaman Arlo U. Landolt James Bedient Karen Jean Meech Gary Billings Christopher Watson Pamela Gay Douglas L. Welch ISSN 0271-9053 JAAVSO The Journal of The American Association of Variable Star Observers Volume 36 Number 1 2008 49 Bay State Road Cambridge, MA 02138 ISSN 0271-9053 U. -
Milestone Goto-Bino Series .Cdr
Kson MilestoneK Standard Alt/Az GOTO Mount INSTRUCTIONS CONTENT FOR KSON STANDARD ALT/AZ GOTO USER INTRODUCTION.................................................................................1 ACCESSORIES..................................................................................2 ASSEMBLY INSTRUCTIONS.............................................................3 FEATURES.........................................................................5 OPERATION MANUAL FOR SKYTOUCH CONTROLLER............... 6 KEY DESCRIPTION.................................................................................6 STATUS DESCRIPTION...........................................................................6 OPERATION PROCESS...........................................................................7 POWER ON......................................................................................7 WARNING........................................................................................7 ALIGNMENT STATUS........................................................................7 CHANGE THE DATE..................................................................7 CHANGE THE TIME...................................................................8 CHANGE THE SITE...................................................................8 ALIGNMENT.............................................................................9 NAVIGATION STATUS.....................................................................11 MENU STATUS................................................................................11 -
Annual Report of IAU Commission G4 Pulsating Stars 2019
Annual Report of IAU Commission G4 Pulsating Stars 2019 Organizational news This is the first report of the Commission with the recently elected leadership. The President of the Commission is Jaymie Matthews. Róbert Szabó was elected as vice president and he was trusted as acting president. The Organizing Committee members are Victoria Antoci, Jadwiga Daszynska-Daszkiewicz, Joyce Guzik, Daniel Huber, Hiromoto Shibahashi. Notable scientific results Below we present an admittedly subjective and incomplete list of the latest, most important and interesting results on pulsating and oscillating stars: 1. G. Clementini, V. Ripepi, R. Molinaro et al: Gaia Data Release 2. Specific characterization and validation of all-sky Cepheids and RR Lyrae stars, A&A, 622, A60, 2019 All-sky sample of selected Cepheids and RR Lyrae stars is analyzed, over 50 000 of which (1/3 of the sample) are new discoveries. 2. Gaia collaboration, L. Eyer, L. Rimoldini et al: Gaia Data Release 2. Variable stars in the colour-absolute magnitude diagram, A&A 623, A110, 2019 This is the most complete description of the colour-absolute magnitude diagram and its variability induced changes based on variable (including pulsating) stars using Gaia DR2. 3-4. P. Kervella, A. Gallenne, N. R. Evans et al: Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2. I & II, A&A 623, A116-A117, 2019 Binarity established from proper motion anomaly and based on common proper motion pairs is investigated in these classical pulsating stars using Gaia DR2 data. 5. W. Chaplin, A. M. Serenelli, A. Miglio et al.: Age dating of an early Milky Way merger via asteroseismology of the naked-eye star nu Indi, Nature Astronomy, 4, 382, 2020 This pioneering work demonstrates how to put constraints on an ancient galactic collision by using asteroseismic age dating of a single bright star observed by TESS. -
Theory of Stellar Atmospheres
© Copyright, Princeton University Press. No part of this book may be distributed, posted, or reproduced in any form by digital or mechanical means without prior written permission of the publisher. EXTENDED BIBLIOGRAPHY References [1] D. Abbott. The terminal velocities of stellar winds from early{type stars. Astrophys. J., 225, 893, 1978. [2] D. Abbott. The theory of radiatively driven stellar winds. I. A physical interpretation. Astrophys. J., 242, 1183, 1980. [3] D. Abbott. The theory of radiatively driven stellar winds. II. The line acceleration. Astrophys. J., 259, 282, 1982. [4] D. Abbott. The theory of radiation driven stellar winds and the Wolf{ Rayet phenomenon. In de Loore and Willis [938], page 185. Astrophys. J., 259, 282, 1982. [5] D. Abbott. Current problems of line formation in early{type stars. In Beckman and Crivellari [358], page 279. [6] D. Abbott and P. Conti. Wolf{Rayet stars. Ann. Rev. Astr. Astrophys., 25, 113, 1987. [7] D. Abbott and D. Hummer. Photospheres of hot stars. I. Wind blan- keted model atmospheres. Astrophys. J., 294, 286, 1985. [8] D. Abbott and L. Lucy. Multiline transfer and the dynamics of stellar winds. Astrophys. J., 288, 679, 1985. [9] D. Abbott, C. Telesco, and S. Wolff. 2 to 20 micron observations of mass loss from early{type stars. Astrophys. J., 279, 225, 1984. [10] C. Abia, B. Rebolo, J. Beckman, and L. Crivellari. Abundances of light metals and N I in a sample of disc stars. Astr. Astrophys., 206, 100, 1988. [11] M. Abramowitz and I. Stegun. Handbook of Mathematical Functions. (Washington, DC: U.S. Government Printing Office), 1972. -
VSS Newsletter – May 2010
Newsletter 2010/2 2010 May From the Director NACAA and the FUTURE Thomas Richards [email protected] Variable star enthusiasts were well represented amongst the hundred-plus attendees at the NACAA conference at Canberra this Easter. Well organised and with high quality pa- pers and posters, it was altogether an exhilarating few days. The theme was "Amateur Astronomy in the Online Age". David Benn started things rolling with a workshop "Variable Star Data Visualisation and Analysis with Vstar". His Vstar software is being developed under contract to AAVSO for online use in the CitizenSky programme - and is already available there. The confer- ence paper sessions kicked off on Saturday morning with the first John Perdrix Address (John founded NACAA) by myself. More of this below. Variable star papers in the con- ference were: Tom Richards: Opportunities and Plans: the Directions of Southern Hemisphere Variable Star Research Alan Plummer: Variable Stars: Observing Stellar Evolution David O'Driscoll: Robotic Research for the Amateur Astronomer Simon O'Toole: The Ubiquity of Exoplanets Tom Richards: Round-table - Variable Stars Planning Session INDEX From the Director Tom Richards 1 Editor’s Comments Stan Walker 3 Stars of the Month Stan Walker 4 Stars That Go Out Stephen Hovell/Stan Walker 5 The Dual Maxima Mira Project Stan Walker 7 The ESP Bug Phil Evans 8 Remarks on Two Possible Cataclysmic Variables Mati Morel 14 CCD Notes—What is the Time on the Sun Tom Richards 16 Here and There 18 Eclipsing Binaries for Fun and Profit—Part IV Bob Nelson 19 The Bright Cepheid Project Stan Walker 31 V1243 Aquilae—A Remarkable Alignment Tom Richards 32 Contact Information 37 It's good to report that David O'Driscoll won the Astral Award for the best presentation.