Stellar Evolution Observing Program
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CO Multi-Line Imaging of Nearby Galaxies (COMING) IV. Overview Of
Publ. Astron. Soc. Japan (2018) 00(0), 1–33 1 doi: 10.1093/pasj/xxx000 CO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project Kazuo SORAI1, 2, 3, 4, 5, Nario KUNO4, 5, Kazuyuki MURAOKA6, Yusuke MIYAMOTO7, 8, Hiroyuki KANEKO7, Hiroyuki NAKANISHI9 , Naomasa NAKAI4, 5, 10, Kazuki YANAGITANI6 , Takahiro TANAKA4, Yuya SATO4, Dragan SALAK10, Michiko UMEI2 , Kana MOROKUMA-MATSUI7, 8, 11, 12, Naoko MATSUMOTO13, 14, Saeko UENO9, Hsi-An PAN15, Yuto NOMA10, Tsutomu, T. TAKEUCHI16 , Moe YODA16, Mayu KURODA6, Atsushi YASUDA4 , Yoshiyuki YAJIMA2 , Nagisa OI17, Shugo SHIBATA2, Masumichi SETA10, Yoshimasa WATANABE4, 5, 18, Shoichiro KITA4, Ryusei KOMATSUZAKI4 , Ayumi KAJIKAWA2, 3, Yu YASHIMA2, 3, Suchetha COORAY16 , Hiroyuki BAJI6 , Yoko SEGAWA2 , Takami TASHIRO2 , Miho TAKEDA6, Nozomi KISHIDA2 , Takuya HATAKEYAMA4 , Yuto TOMIYASU4 and Chey SAITA9 1Department of Physics, Faculty of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo 060-0810, Japan 2Department of Cosmosciences, Graduate School of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo 060-0810, Japan 3Department of Physics, School of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo 060-0810, Japan 4Division of Physics, Faculty of Pure and Applied Sciences, University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8571, Japan 5Tomonaga Center for the History of the Universe (TCHoU), University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8571, Japan 6Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, -
136, June 2008
British Astronomical Association VARIABLE STAR SECTION CIRCULAR No 136, June 2008 Contents Group Photograph, AAVSO/BAAVSS meeting ........................ inside front cover From the Director ............................................................................................... 1 Eclipsing Binary News ....................................................................................... 4 Experiments in the use of a DSLR camera for V photometry ............................ 5 Joint Meeting of the AAVSO and the BAAVSS ................................................. 8 Coordinated HST and Ground Campaigns on CVs ............................... 8 Eclipsing Binaries - Observational Challenges .................................................. 9 Peer to Peer Astronomy Education .................................................................. 10 AAVSO Acronyms De-mystified in Fifteen Minutes ...................................... 11 New Results on SW Sextantis Stars and Proposed Observing Campaign ........ 12 A Week in the Life of a Remote Observer ........................................................ 13 Finding Eclipsing Binaries in NSVS Data ......................................................... 13 British Variable Star Associations 1848-1908 .................................................. 14 “Chasing Rainbows” (The European Amateur Spectroscopy Scene) .............. 15 Long Term Monitoring and the Carbon Miras ................................................. 18 Cataclysmic Variables from Large Surveys: A Silent Revolution -
Cassiopeia A: on the Origin of the Hard X-Ray Continuum and the Implication of the Observed O Vııı Ly-Α/Ly-Β Distribution
A&A 365, L225–L230 (2001) Astronomy DOI: 10.1051/0004-6361:20000048 & c ESO 2001 Astrophysics Cassiopeia A: On the origin of the hard X-ray continuum and the implication of the observed O vııı Ly-α/Ly-β distribution J. A. M. Bleeker1, R. Willingale2, K. van der Heyden1, K. Dennerl3,J.S.Kaastra1, B. Aschenbach3, and J. Vink4,5,6 1 SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands 2 Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK 3 Max-Planck-Institut f¨ur extraterrestrische Physik, Giessenbachstraße, 85740 Garching, Germany 4 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany 5 Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA 6 Chandra Fellow Received 6 October 2000 / Accepted 24 October 2000 Abstract. We present the first results on the hard X-ray continuum image (up to 15 keV) of the supernova remnant Cas A measured with the EPIC cameras onboard XMM-Newton. The data indicate that the hard X-ray tail, observed previously, that extends to energies above 100 keV does not originate in localised regions, like the bright X-ray knots and filaments or the primary blast wave, but is spread over the whole remnant with a rather flat hardness ratio of the 8–10 and 10–15 keV energy bands. This result does not support an interpretation of the hard X-radiation as synchrotron emission produced in the primary shock, in which case a limb brightened shell of hard X-ray emission close to the primary shock front is expected. -
The Extragalactic Distance Scale
The Extragalactic Distance Scale Published in "Stellar astrophysics for the local group" : VIII Canary Islands Winter School of Astrophysics. Edited by A. Aparicio, A. Herrero, and F. Sanchez. Cambridge ; New York : Cambridge University Press, 1998 Calibration of the Extragalactic Distance Scale By BARRY F. MADORE1, WENDY L. FREEDMAN2 1NASA/IPAC Extragalactic Database, Infrared Processing & Analysis Center, California Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA 91125, USA 2Observatories, Carnegie Institution of Washington, 813 Santa Barbara St., Pasadena CA 91101, USA The calibration and use of Cepheids as primary distance indicators is reviewed in the context of the extragalactic distance scale. Comparison is made with the independently calibrated Population II distance scale and found to be consistent at the 10% level. The combined use of ground-based facilities and the Hubble Space Telescope now allow for the application of the Cepheid Period-Luminosity relation out to distances in excess of 20 Mpc. Calibration of secondary distance indicators and the direct determination of distances to galaxies in the field as well as in the Virgo and Fornax clusters allows for multiple paths to the determination of the absolute rate of the expansion of the Universe parameterized by the Hubble constant. At this point in the reduction and analysis of Key Project galaxies H0 = 72km/ sec/Mpc ± 2 (random) ± 12 [systematic]. Table of Contents INTRODUCTION TO THE LECTURES CEPHEIDS BRIEF SUMMARY OF THE OBSERVED PROPERTIES OF CEPHEID -
METEOR CSILLAGÁSZATI ÉVKÖNYV 2019 Meteor Csillagászati Évkönyv 2019
METEOR CSILLAGÁSZATI ÉVKÖNYV 2019 meteor csillagászati évkönyv 2019 Szerkesztette: Benkő József Mizser Attila Magyar Csillagászati Egyesület www.mcse.hu Budapest, 2018 Az évkönyv kalendárium részének összeállításában közreműködött: Tartalom Bagó Balázs Görgei Zoltán Kaposvári Zoltán Kiss Áron Keve Kovács József Bevezető ....................................................................................................... 7 Molnár Péter Sánta Gábor Kalendárium .............................................................................................. 13 Sárneczky Krisztián Szabadi Péter Cikkek Szabó Sándor Szőllősi Attila Zsoldos Endre: 100 éves a Nemzetközi Csillagászati Unió ........................191 Zsoldos Endre Maria Lugaro – Kereszturi Ákos: Elemkeletkezés a csillagokban.............. 203 Szabó Róbert: Az OGLE égboltfelmérés 25 éve ........................................218 A kalendárium csillagtérképei az Ursa Minor szoftverrel készültek. www.ursaminor.hu Beszámolók Mizser Attila: A Magyar Csillagászati Egyesület Szakmailag ellenőrizte: 2017. évi tevékenysége .........................................................................242 Szabados László Kiss László – Szabó Róbert: Az MTA CSFK Csillagászati Intézetének 2017. évi tevékenysége .........................................................................248 Petrovay Kristóf: Az ELTE Csillagászati Tanszékének működése 2017-ben ............................................................................ 262 Szabó M. Gyula: Az ELTE Gothard Asztrofi zikai Obszervatórium -
Events: General Meeting : No General Meeting This Month
The monthly newsletter of the Temecula Valley Astronomers July 2016 Events: General Meeting : No general meeting this month. Join us for our annual Anza Star-B-Q. Watch your email for details. For the latest on Star Parties, check the web page. Juno spacecraft and its science instruments. Image credit: NASA/JPL General information: Subscription to the TVA is included in the annual $25 WHAT’S INSIDE THIS MONTH: membership (regular members) donation ($9 student; $35 family). Cosmic Comments by President Mark Baker President: Mark Baker 951-691-0101 Looking Up <[email protected]> Vice President: Chuck Dyson <[email protected]> by Curtis Croulet Past President: John Garrett <[email protected]> Random thoughts Treasurer: Curtis Croulet <[email protected]> by Chuck Dyson Secretary: Deborah Cheong <[email protected]> Hubble's bubble lights up the Club Librarian: Bob Leffler <[email protected]> interstellar rubble Facebook: Tim Deardorff <[email protected]> Star Party Coordinator and Outreach: Deborah Cheong by Ethan Siegel <[email protected]> Send newsletter submissions to Mark DiVecchio Address renewals or other correspondence to: <[email protected]> by the 20th of the month for Temecula Valley Astronomers the next month's issue. PO Box 1292 Murrieta, CA 92564 Like us on Facebook Member’s Mailing List: [email protected] Website: http://www.temeculavalleyastronomers.com/ Page 1 of 10 The monthly newsletter of the Temecula Valley Astronomers July 2016 Cosmic Comments – July/2016 by President Mark Baker As some of you may notice, I will often despair at the current state of the US Space program, to the point of disparagement. -
A Csillagképek Története És Látnivalói, 2019. Március 13
Az északi pólus környéke 2. A csillagképek története és látnivalói, 2019. március 13. Sárkány • Latin: Draco, birtokos: Draconis, rövidítés: Dra • Méretbeli rangsor: 8. (1083°2, a teljes égbolt 2,63%-a) 2m 3m 4m 5m 6m • Eredet: görög (Δράκων (Drakón)) 1 5 10 57 144 Cefeusz Kis Medve Kultúrtörténet Görögök: kígyó (korábban) v. sárkány • ő Ladón, a Heszperiszek Kertjének őre: itt található Héra nászajándéka, egy örök ifjúságot és halhatatlanságot adó aranyalmákat érlelő fa • Héraklész 10+1-edik feladatként ellopott három almát • vagy ő maga, mérgezett nyilakkal elpusztítva Ladónt • vagy megkérte erre Atlaszt, és addig tartotta helyette az eget Héraklész rálép a sárkány • Héra emlékül az égre helyezte fejére (Dürer) Arabok • a sárkányfej-négyszöget (, , , ) 4 anyatevének látták • akik egy teveborjút védelmeznek (?) • mert azt két hiéna (, ) támadja • a tevék gazdái (, , ) a közelben táboroznak Kína • a Központi Palotát közrefogó két „fal” nagy része itt futott • Csillagok: semmi nagyon extra • Az É-i ekliptikai pólus ide esik • Az É-i pólus -3000 környékén az Dra (Thuban) közelébe esett • Mélyég: Macskaszem-köd (NGC 6543): planetáris köd: haldokló óriáscsillag által ledobott anyagfelhő A Kéfeusz-Kassziopeia-Androméda • Kéfeusz Etiópia királya, Zeusz leszármazottja (egyik szeretője, Io jóvoltából) mondakör • felesége, Kassziopeia annyira hiú volt a saját vagy a lánya szépségére („szebb, mint a nereidák”), hogy Poszeidón egy tengeri szörnyet (Cet) küldött büntetésből a királyság pusztítására • hogy elhárítsák a veszedelmet, egy jós tanácsára -
PDF Version in Chronological Order (Updated May 17, 2013)
Complete Bibliography for Ritter Observatory May 17, 2013 The following papers are based in whole or in part on observations made at Ritter Observatory. External collaborators are listed in parentheses unless the research was done while they were University of Toledo students. Refereed or invited: 1. A. H. Delsemme and J. L. Moreau 1973, Astrophys. Lett., 14, 181–185, “Brightness Profiles in the Neutral Coma of Comet Bennett (1970 II)” 2. B. W. Bopp and F. Fekel Jr. 1976, A. J., 81, 771–773, “HR 1099: A New Bright RS CVn Variable” 3. A. H. Delsemme and M. R. Combi 1976, Ap. J. (Letters), 209, L149–L151, “The Production Rate and Possible Origin of O(1D) in Comet Bennett 1970 II” 4. A. H. Delsemme and M. R. Combi 1976, Ap. J. (Letters), 209, L153–L156, “Production + Rate and Origin of H2O in Comet Bennett 1970 II” 5. D. W. Willmarth 1976, Pub. A. S. P., 88, 86–87, “The Orbit of 71 Draconis” 6. W. F. Rush and R. W. Thompson 1977, Ap. J., 211, 184–188, “Rapid Variations of Emission-Line Profiles in Nova Cygni 1975” 7. S. E. Smith and B. W. Bopp 1980, Pub. A. S. P., 92, 225–232, “A Microcomputer-Based System for the Automated Reduction of Astronomical Spectra” 8. B. W. Bopp and P. V. Noah 1980, Pub. A. S. P., 92, 333–337, “Spectroscopic Observations of the Surface-Activity Binary II Pegasi (HD 224085)” 9. M. R. Combi and A. H. Delsemme 1980, Ap. J., 237, 641–645, “Neutral Cometary Atmospheres. II. -
Blasts from the Past Historic Supernovas
BLASTS from the PAST: Historic Supernovas 185 386 393 1006 1054 1181 1572 1604 1680 RCW 86 G11.2-0.3 G347.3-0.5 SN 1006 Crab Nebula 3C58 Tycho’s SNR Kepler’s SNR Cassiopeia A Historical Observers: Chinese Historical Observers: Chinese Historical Observers: Chinese Historical Observers: Chinese, Japanese, Historical Observers: Chinese, Japanese, Historical Observers: Chinese, Japanese Historical Observers: European, Chinese, Korean Historical Observers: European, Chinese, Korean Historical Observers: European? Arabic, European Arabic, Native American? Likelihood of Identification: Possible Likelihood of Identification: Probable Likelihood of Identification: Possible Likelihood of Identification: Possible Likelihood of Identification: Definite Likelihood of Identification: Definite Likelihood of Identification: Possible Likelihood of Identification: Definite Likelihood of Identification: Definite Distance Estimate: 8,200 light years Distance Estimate: 16,000 light years Distance Estimate: 3,000 light years Distance Estimate: 10,000 light years Distance Estimate: 7,500 light years Distance Estimate: 13,000 light years Distance Estimate: 10,000 light years Distance Estimate: 7,000 light years Distance Estimate: 6,000 light years Type: Core collapse of massive star Type: Core collapse of massive star Type: Core collapse of massive star? Type: Core collapse of massive star Type: Thermonuclear explosion of white dwarf Type: Thermonuclear explosion of white dwarf? Type: Core collapse of massive star Type: Thermonuclear explosion of white dwarf Type: Core collapse of massive star NASA’s ChANdrA X-rAy ObServAtOry historic supernovas chandra x-ray observatory Every 50 years or so, a star in our Since supernovas are relatively rare events in the Milky historic supernovas that occurred in our galaxy. Eight of the trine of the incorruptibility of the stars, and set the stage for observed around 1671 AD. -
The Stellar Populacons of IC 10 and NGC 1569 Observed with Keck
The Stellar Populaons of IC 10 and NGC 1569 observed with Keck LGSAO and HST William D. Vacca (USRA‐SOFIA) Chris Sheehy James Graham (UC Berkeley) Nate McCrady (UCLA) Properes of IC 10 • Small irregular starburst (BCD) galaxy on outskirts of Local Group – R ~ 1 kpc 9 – M ~ 1‐2 x 10 M • Low metallicity (Z ~ 0.2‐0.3 Z~ ZSMC) • Brief, galaxy‐wide burst of SF occurred within last 10 Myr – Numerous HII regions – Large Hα and FIR luminosity ‐1 • Highest SFR of any LG dwarf (> 0.7 M yr ) – Large populaon of W‐R stars (NWR > 24; SMC has ~ 8) • Highest surface density of W‐Rs in LG ( ~ 8 kpc‐2; MW ~ 2.5 kpc‐2) • Anomalously high WC/WN rao ( ~ 1‐2) for its Z (10x too large!) • Have WN stars been missed in surveys? • b = −3.3° – Uncertain reddening: AV = 1.2 – 6.0 mag – Uncertain distance: D = 0.5 – 3.0 Mpc • Ideal extragalacc target for NIR observaons with LGSAO – Nearby, relavely large AV (foreground and internal), high ρ★ – Bright p‐lt guide stars available N IC 10 HST/ACS/WFC F435W, F606W, F814W 1” ≈ 4 pc WR Object: [MAC92] 24 • Brightest W‐R candidate in HST/WFPC2 F555W IC10 • Lies within prominent H II region HL 111c • Lies at center of a young stellar cluster (Hunter 2001) • Uncertain spectral type 5’’ – Weak, broad He II 4686 emission (Massey & Holmes 2002) – WN+OB? • Three components (A, B, C) • Cluster itself? Crowther et al. (2003) Observaons • NIR Data: • Opcal Data: – NIRC2/Keck II/LGSAO H and K’ – HST/ACS/WFC F814W – 0.01”pixel‐1 – 0.05”pixel‐1 – Final FOV = 12.2” x 12.2” – texp = 1080 s – texp = 1200 s (H); 1500 s (K’) – FWHM = 0.08” – FWHM = 0.048” (H); 0.051” (K’) – Strehl ~ 18% (H); 32% (K’) ACS WFC / NIRC2 Comparison HST/ACS/WFC F814W Keck II/NIRC2/LGSAO K’ IC 10 IHK’ N E 12.2” x 12.2” 47 pc x 47 pc Vacca, Sheehy, & Graham (2007) CMD of IC 10 [MAC92] 24 Region Opcal Data: • PSF fing (Anderson & King 2006) • 690 stars found in F814W • [F814W]Lim ~ 25.25 • σ < 0.04 mag for [F814W] < 23.0 NIR Data: • MTF‐fing method (Sheehy et al. -
Variable Star Section Circular
ΒΑΛ The British Astronomical Association VARIABLE STAR SECTION CIRCULAR 64 "LIGHT-CURVE” AUGUST 1986 ISSN 0267-9272 Office: Burlington House, Piccadilly, London, W1V 9AG SECTION OFFICERS: Director D.R.B. Saw, 'Upanova1, 18 Dolllcott, Haddenham, Aylesbury, Bucks. HP17 8JG Tel: Haddenham (0844) 292065 Assistant Director S.R. Dunlop, 140 Stocks Lane, East Wittering, nr Chichester, West Sussex P020 8NT Tel: Bracklesham Bay (0243) 670354 Secretary M.D. Taylor, 17 Cross Lane, Wakefield, West Yorkshire WF2 8DA Tel: Wakefield (0924) 374651 Programme Secretaries: Assistant Secretary (Post temporarily vacant) Telescopic Assistant Secretary J. Toone, 2 Hilton Crescent, Boothstown, Binocular Worsley, Manchester M28 4FY Tel: 061 702 8619 Eclipsing Binary J.E. Isles, Rose Cottage, 22 High Street, Secretary Wescott, Bucks. HP18 OPU Tel: Aylesbury (0296) 651779 Nova/Supernova G.M Hurst, 16 Westminster Close, Search Secretary Kempshott Rise, Basingstoke, Hants. RG22 4PP Tel: Basingstoke (0256) 471074 Chart Secretary J. Parkinson, 229 Scar Lane, Golcar, (except Eclipsing) Huddersfield, West Yorkshire HD7 4AU Tel: Huddersfield (0484) 642947 For subcription rates and charges for charts and other publications see inside back cover. Editorial It has been suggested that these C irc u la rs are often a little 'dry' and technical for some members. We are always happy to receive more 'personal' items and hope to include more in future issues. We are also including an occasional short note on some of the terms encountered, and which may not be fully explained in some of the specific articles. The first such item appears on p.13. If you have any queries, however elementary, please send them in, and we shall do our best to provide the answers. -
Introduction to Astronomical Photometry, Second Edition
This page intentionally left blank Introduction to Astronomical Photometry, Second Edition Completely updated, this Second Edition gives a broad review of astronomical photometry to provide an understanding of astrophysics from a data-based perspective. It explains the underlying principles of the instruments used, and the applications and inferences derived from measurements. Each chapter has been fully revised to account for the latest developments, including the use of CCDs. Highly illustrated, this book provides an overview and historical background of the subject before reviewing the main themes within astronomical photometry. The central chapters focus on the practical design of the instruments and methodology used. The book concludes by discussing specialized topics in stellar astronomy, concentrating on the information that can be derived from the analysis of the light curves of variable stars and close binary systems. This new edition includes numerous bibliographic notes and a glossary of terms. It is ideal for graduate students, academic researchers and advanced amateurs interested in practical and observational astronomy. Edwin Budding is a research fellow at the Carter Observatory, New Zealand, and a visiting professor at the Çanakkale University, Turkey. Osman Demircan is Director of the Ulupınar Observatory of Çanakkale University, Turkey. Cambridge Observing Handbooks for Research Astronomers Today’s professional astronomers must be able to adapt to use telescopes and interpret data at all wavelengths. This series is designed to provide them with a collection of concise, self-contained handbooks, which covers the basic principles peculiar to observing in a particular spectral region, or to using a special technique or type of instrument. The books can be used as an introduction to the subject and as a handy reference for use at the telescope, or in the office.