Annual Report 2011
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Explore the Universe Observing Certificate Second Edition
RASC Observing Committee Explore the Universe Observing Certificate Second Edition Explore the Universe Observing Certificate Welcome to the Explore the Universe Observing Certificate Program. This program is designed to provide the observer with a well-rounded introduction to the night sky visible from North America. Using this observing program is an excellent way to gain knowledge and experience in astronomy. Experienced observers find that a planned observing session results in a more satisfying and interesting experience. This program will help introduce you to amateur astronomy and prepare you for other more challenging certificate programs such as the Messier and Finest NGC. The program covers the full range of astronomical objects. Here is a summary: Observing Objective Requirement Available Constellations and Bright Stars 12 24 The Moon 16 32 Solar System 5 10 Deep Sky Objects 12 24 Double Stars 10 20 Total 55 110 In each category a choice of objects is provided so that you can begin the certificate at any time of the year. In order to receive your certificate you need to observe a total of 55 of the 110 objects available. Here is a summary of some of the abbreviations used in this program Instrument V – Visual (unaided eye) B – Binocular T – Telescope V/B - Visual/Binocular B/T - Binocular/Telescope Season Season when the object can be best seen in the evening sky between dusk. and midnight. Objects may also be seen in other seasons. Description Brief description of the target object, its common name and other details. Cons Constellation where object can be found (if applicable) BOG Ref Refers to corresponding references in the RASC’s The Beginner’s Observing Guide highlighting this object. -
A Dynamo Mechanism As the Potential Origin of the Long Cycle in Double Periodic Variables Dominik R
A&A 602, A109 (2017) Astronomy DOI: 10.1051/0004-6361/201628900 & c ESO 2017 Astrophysics A dynamo mechanism as the potential origin of the long cycle in double periodic variables Dominik R. G. Schleicher and Ronald E. Mennickent Departamento de Astronomía, Facultad Ciencias Físicas y Matemáticas, Universidad de Concepción, Av. Esteban Iturra s/n Barrio Universitario, Casilla 160-C, Concepción, Chile e-mail: [email protected] Received 11 May 2016 / Accepted 9 March 2017 ABSTRACT The class of double period variables (DPVs) consists of close interacting binaries, with a characteristic long period that is an order of magnitude longer than the corresponding orbital period, many of them with a characteristic ratio of approximately 35. We consider here the possibility that the accretion flow is modulated as a result of a magnetic dynamo cycle. Due to the short binary separations, we expect the rotation of the donor star to be synchronized with the rotation of the binary due to tidal locking. We here present a model to estimate the dynamo number and the resulting relation between the activity cycle length and the orbital period, as well as an estimate for the modulation of the mass transfer rate. The latter is based on Applegate’s scenario, implying cyclic changes in the radius of the donor star and thus in the mass transfer rate as a result of magnetic activity. Our model is applied to a sample of 17 systems with known physical parameters, 11 of which also have known modulation periods. In spite of the uncertainties of our simplified framework, the results show a reasonable agreement, indicating that a dynamo interpretation is potentially feasible. -
Annual Report 2010
Research Institute Leiden Observatory (Onderzoekinstituut Sterrewacht Leiden) Annual Report 2010 Sterrewacht Leiden Faculty of Mathematics and Natural Sciences Leiden University Niels Bohrweg 2 Postbus 9513 2333 CA Leiden 2330 RA Leiden The Netherlands http://www.strw.leidenuniv.nl Cover: In the Sackler Laboratory for Astrophysics, the circumstances in the inter- and circumstellar medium are simulated. In 2010, water was successfully made on icy dust grains by H-atom bombardment, understanding was gained how complex molecules form under the extreme conditions that are typical for space, and experiments are now ongoing that investigate under which conditions the building blocks of life form. The picture shows the lab’s newest setup - MATRI2CES - that has been constructed with the aim to 'unlock the chemistry of the heavens'. An electronic version of this annual report is available on the web at http://www.strw.leidenuniv.nl/research/annualreport.php?node=23 Production Annual Report 2010: A. van der Tang, E. Gerstel, F.P. Israel, J. Lub, M. Israel, E. Deul Sterrewacht Leiden Executive (Directie Onderzoeksinstituut) Director K. Kuijken Wetenschappelijk Directeur Director of Education F.P. Israel Onderwijs Directeur Institute Manager E. Gerstel Instituutsmanager Supervisory Council (Raad van advies) Prof. Dr. Ir. J.A.M. Bleeker (Chair) Dr. B. Baud Drs. J.F. van Duyne Prof. Dr. K. Gaemers Prof. Dr. C. Waelkens CONTENTS Contents: Part I Chapter 1 1.1 Foreword 1 1.2 Obituary Adriaan Blaauw 5 1.3 Obituary Jaap Tinbergen 7 Chapter 2 2.1 Heritage 11 2.2 Extrasolar planets 13 2.3 Circumstellar gas and dust 15 2.4 Chemistry and physics of the interstellar medium 20 2.5 Stars 25 2.6 Galaxies of the Local Group 30 2.7 Nearby galaxies: observations and theory 37 2.8. -
Abstracts of Talks 1
Abstracts of Talks 1 INVITED AND CONTRIBUTED TALKS (in order of presentation) Milky Way and Magellanic Cloud Surveys for Planetary Nebulae Quentin A. Parker, Macquarie University I will review current major progress in PN surveys in our own Galaxy and the Magellanic clouds whilst giving relevant historical context and background. The recent on-line availability of large-scale wide-field surveys of the Galaxy in several optical and near/mid-infrared passbands has provided unprecedented opportunities to refine selection techniques and eliminate contaminants. This has been coupled with surveys offering improved sensitivity and resolution, permitting more extreme ends of the PN luminosity function to be explored while probing hitherto underrepresented evolutionary states. Known PN in our Galaxy and LMC have been significantly increased over the last few years due primarily to the advent of narrow-band imaging in important nebula lines such as H-alpha, [OIII] and [SIII]. These PNe are generally of lower surface brightness, larger angular extent, in more obscured regions and in later stages of evolution than those in most previous surveys. A more representative PN population for in-depth study is now available, particularly in the LMC where the known distance adds considerable utility for derived PN parameters. Future prospects for Galactic and LMC PN research are briefly highlighted. Local Group Surveys for Planetary Nebulae Laura Magrini, INAF, Osservatorio Astrofisico di Arcetri The Local Group (LG) represents the best environment to study in detail the PN population in a large number of morphological types of galaxies. The closeness of the LG galaxies allows us to investigate the faintest side of the PN luminosity function and to detect PNe also in the less luminous galaxies, the dwarf galaxies, where a small number of them is expected. -
Free Astronomy Magazine May-June 2020
cover EN.qxp_l'astrofilo 27/04/2020 16:36 Page 1 THE FREE MULTIMEDIA MAGAZINE THAT KEEPS YOU UPDATED ON WHAT IS HAPPENING IN SPACE Bi-monthly magazine of scientific and technical information ✶ May-June 2020 BBiioofflluuoorreesscceenntt ppllaanneetsts The star S2 moves according to Einstein’s Relativity Do sub-relativistic meteors exist? www.astropublishing.com ✶✶www.facebook.com/astropublishing [email protected] colophon EN_l'astrofilo 27/04/2020 16:36 Page 2 colophon EN_l'astrofilo 27/04/2020 16:36 Page 3 S U M M A R Y BI-MONTHLY MAGAZINE OF SCIENTIFIC AND TECHNICAL INFORMATION The star S2 moves according to Einstein’s Relativity FREELY AVAILABLE THROUGH Observations made with ESO’s Very Large Telescope (VLT) have revealed for the first time that a star or- THE INTERNET biting the supermassive black hole at the centre of the Milky Way moves just as predicted by Einstein’s general theory of relativity. Its orbit is shaped like a rosette and not like an ellipse as predicted by... May-June 2020 4 Biofluorescent planets The closest potentially habitable rocky exoplanets all orbit around red dwarfs. These types of stars are particularly suitable for hosting Earth-sized planets, but they are also characterized by surface phenom- 10 ena very harmful to life as we know it. Some organisms, however, may be able to adapt to intense... ESO telescope observes exoplanet where it rains iron Researchers using ESO’s Very Large Telescope (VLT) have observed an extreme planet where they suspect it rains iron. The ultra-hot giant exoplanet has a day side where temperatures climb above 2400 degrees 22 Celsius, high enough to vaporise metals. -
Adrian Zielonka's December Space and Astronomy News
Adrian Zielonka’s Astronomy and Space News Night Sky 2018 - December Sunrise Sunset Mercury Rises Venus Rises st st st st 1 – 7:52am 1 – 4:07pm 1 – 6:59am 1 – 4:10am th th th th 10 – 8:03am 10 – 4:04pm 10 – 6:10am 10 – 4:02am th th th th 20 – 8:11am 20 – 4:06pm 20 – 6:26am 20 – 4:03am th th th th 30 – 8:15am 30 – 4:13pm 30 – 7:03am 30 – 4:13am Moon Rise Moon Set Moon Rise Moon Set st st th th 1 – 12:34am 1 – 1:55pm 16 – 1:12pm 17 – 1:24am nd nd th th 2 – 1:50am 2 – 2:18pm 17 – 1:32pm 18 – 2:34am rd rd th th 3 – 3:04am 3 – 2:40pm 18 – 1:54pm 19 – 3:47am th th th th 4 – 4:18am 4 – 3:04pm 19 – 2:19pm 20 – 5:02am th th th st 5 – 5:30am 5 – 3:30pm 20 – 2:48pm 21 – 6:18am th th st nd 6 – 6:41am 6 – 4:00pm 21 – 3:26pm 22 – 7:33am (Full) th th nd rd 7 – 7:48am (New) 7 – 4:35pm (New) 22 – 4:13pm (Full) 23 – 8:42am th th rd th 8 – 8:49am 8 – 5:17pm 23 – 5:12pm 24 – 9:41am th th th th 9 – 9:44am 9 – 6:06pm 24 – 6:23pm 25 – 10:28am th th th th 10 – 10:30am 10 – 7:00pm 25 – 7:41pm 26 – 11:05am th th th th 11 – 11:08am 11 – 8:00pm 26 – 9:01pm 27 – 11:36am th th th th 12 – 11:40am 12 – 9:02pm 27 – 10:21pm 28 – 12:02pm th th th th 13 – 12:07pm 13 – 10:06pm 28 – 11:39pm 29 – 12:25pm (LQ) th th th th 14 – 12:30pm 14 – 11:11pm 30 – 12:54am 30 – 12:47pm th th st st 15 – 12:52pm (FQ) 16 – 12:17am 31 – 2:08am 31 – 1:10pm A useful site: www.heavens- above.com A S Zielonka There is a planned launch this month of a Chinese Long March 2D rocket from Jiuquan Satellite Launch Center, China. -
Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem
Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. Linee guide per l’utilizzo Google è orgoglioso di essere il partner delle biblioteche per digitalizzare i materiali di pubblico dominio e renderli universalmente disponibili. I libri di pubblico dominio appartengono al pubblico e noi ne siamo solamente i custodi. Tuttavia questo lavoro è oneroso, pertanto, per poter continuare ad offrire questo servizio abbiamo preso alcune iniziative per impedire l’utilizzo illecito da parte di soggetti commerciali, compresa l’imposizione di restrizioni sull’invio di query automatizzate. Inoltre ti chiediamo di: + Non fare un uso commerciale di questi file Abbiamo concepito Google Ricerca Libri per l’uso da parte dei singoli utenti privati e ti chiediamo di utilizzare questi file per uso personale e non a fini commerciali. -
NRAO Newsletter
NRAONRAO NewsletterNewsletter The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. January 2003 www.nrao.edu/news/newsletters Number 94 ALMA This fall has been a busy period as construction activities a detailed proposal to bring significant enhancements to the accelerate for the ALMA project. The most visible evidence baseline ALMA. These enhancements may include a of progress is the completion of the first prototype antenna compact array of seven- and twelve-meter antennas to at the ALMA Test Facility (ATF) located at the VLA site. improve imaging with short baselines, additional frequency The VertexRSI antenna erection has been completed and the bands, and a second generation correlator. Choices of antenna is undergoing a period of extensive tests to verify enhancements will depend on the level of Japanese funds its performance. A second antenna, supplied by our available. The ALMA Science Advisory Committee European partners, will be erected at the ATF next year. The (ASAC) has provided the ACC with the science cases and a European antenna, produced by a consortium led by the priority ranking of potential ALMA enhancements. In antic- French company Alcatel, is scheduled to be available for ipation of their entry, the Japanese will bring a prototype tests beginning in June 2003. Construction of the founda- antenna to the ATF in 2003 for tests to verify its suitability tion for this antenna is already underway. for use in the compact array. The ALMA Coordinating Committee (ACC) met with NRAO Director Fred Lo has convened a panel of experts the Japanese at ESO headquarters in Germany to begin from inside NRAO to review the technical details of those negotiations for the possible entry of Japan into the ALMA portions of the ALMA project assigned to North America. -
Liste Des Juges
Liste des juges Jean-François VANAKEN (Belgique) Norman DESCHUYMERE (Belgique) Walter VAN DEN BROECK (Belgique) Elisabeth FEUZ (Suisse) Aida RIVERA (Colombie) Juan A. GRILLO (Colombie) Horst KLIEBENSTEIN (Allemagne) Istvan CSIK (Allemagne) Siret LEPASAAR (Estonie) Jean-Jacques MORBELLI (France) Jussi LIIMATAINEN (Finlande) Frank KANE (Royaume-Uni) Roger CROOKS (Royaume-Uni) Ildiko MUZSLAI (Hongrie) Manola POGGESI (Italie) Massimo INZOLI (Italie) Sonia FALLETTI-BELLAN (Italie) Andi HUDONO (Indonésie) Yolanda NAGLER-MAGAL (Israël) Michael LEONARD (Irlande) Gloria WAGNER (Luxembourg) Laurent HEINESCHE (Luxembourg) Ruth WAGNER (Luxembourg) Oystein EIKESETH (Norvège) Wenche EIKESETH (Norvège) Gerard JIPPING (Pays-Bas) John WILLIAMS (Pays-Bas) Zeferino Jose Cardoso SILVA (Portugal) Jan GAJEWSKI (Pologne) Malgorzata HALAS (Pologne) Blaz KAVCIC (Slovénie) Marija KAVCIC (Slovénie) Tatjana UREK (Slovénie) Bratislav MILOSEVIC (Serbie) Ozan BELKIS (Turquie) Donavon THOMPSON (Etats Unis d'Amérique) 90th International Dog Show - Chiens exposés par pays. Pays Nombre Country France 1726 France Allemagne 1102 Deutschland Belgique 857 België Pays-Bas 543 Nederland Espagne 150 España Italie 141 Italia Luxembourg 125 Lëtzebuerg Danemark 100 Danmark Suisse 93 Schweiz Royaume-Uni 87 Great Britain Russie 74 Rossijskaja Federazija République tchèque 60 Ceskà republika Pologne 44 Polska Hongrie 27 Magyarország Ukraine 25 Ykpaïha Irlande 22 Éire Roumanie 15 România Autriche 14 Österreich Suède 13 Sverige Portugal 10 Portugal Norvège 8 Norge Slovénie 8 Slovenija Croatie 8 Hrvatska Lettonie 7 Latvija Serbie 4 Srbija Finlande 4 Suomi Bulgarie 3 Balgarija Slovaquie 3 Slovensko Etats Unis d'Amérique 2 United States of America Estonie 2 Eesti Grèce 2 Elláda Montenegro 1 Crna Gora Lituanie 1 Lietuva Total 5281 Total Race/Breed Ring Chiens/Dogs Groupe F.C.I. -
Astronomy Magazine 2020 Index
Astronomy Magazine 2020 Index SUBJECT A AAVSO (American Association of Variable Star Observers), Spectroscopic Database (AVSpec), 2:15 Abell 21 (Medusa Nebula), 2:56, 59 Abell 85 (galaxy), 4:11 Abell 2384 (galaxy cluster), 9:12 Abell 3574 (galaxy cluster), 6:73 active galactic nuclei (AGNs). See black holes Aerojet Rocketdyne, 9:7 airglow, 6:73 al-Amal spaceprobe, 11:9 Aldebaran (Alpha Tauri) (star), binocular observation of, 1:62 Alnasl (Gamma Sagittarii) (optical double star), 8:68 Alpha Canum Venaticorum (Cor Caroli) (star), 4:66 Alpha Centauri A (star), 7:34–35 Alpha Centauri B (star), 7:34–35 Alpha Centauri (star system), 7:34 Alpha Orionis. See Betelgeuse (Alpha Orionis) Alpha Scorpii (Antares) (star), 7:68, 10:11 Alpha Tauri (Aldebaran) (star), binocular observation of, 1:62 amateur astronomy AAVSO Spectroscopic Database (AVSpec), 2:15 beginner’s guides, 3:66, 12:58 brown dwarfs discovered by citizen scientists, 12:13 discovery and observation of exoplanets, 6:54–57 mindful observation, 11:14 Planetary Society awards, 5:13 satellite tracking, 2:62 women in astronomy clubs, 8:66, 9:64 Amateur Telescope Makers of Boston (ATMoB), 8:66 American Association of Variable Star Observers (AAVSO), Spectroscopic Database (AVSpec), 2:15 Andromeda Galaxy (M31) binocular observations of, 12:60 consumption of dwarf galaxies, 2:11 images of, 3:72, 6:31 satellite galaxies, 11:62 Antares (Alpha Scorpii) (star), 7:68, 10:11 Antennae galaxies (NGC 4038 and NGC 4039), 3:28 Apollo missions commemorative postage stamps, 11:54–55 extravehicular activity -
Binary Star Studies with NPOI
CHARA/NPOI 2013 Science & Technology Review Binary studies with the Navy Precision Optical Interferometer Christian Hummel (ESO) Robert Zavala (USNO), Jason Sanborn (NAU, Lowell) + collaborators CHARA/NPOI 2013 Science & Technology Review Some current projects • Zeta Orionis – 7 year orbit, only recently finished after discovery in 2000 • Sigma Orionis – NPOI’s most “frustrating” target • Xi Tauri – Unknown origin, then “revived” by Petr Harmanec • HR 6493 – Forgotten, then “revived” by Shulin Ren • b Per • delta Lib CHARA/NPOI 2013 Science & Technology Review ζ Ori σ Ori CHARA/NPOI 2013 Science & Technology Review Zeta Orionis Ab B0.5V O9.5I (V=2.0) 40 mas Discovered by Hummel et al. 2000, predicted by Hanbury Brown et al. 1974 CHARA/NPOI 2013 Science & Technology Review The orbit after 7 years CHARA/NPOI 2013 Science & Technology Review Spectroscopy and radial velocities CHARA/NPOI 2013 Science & Technology Review Radial velocity fitting CHARA/NPOI 2013 Science & Technology Review System parameters CHARA/NPOI 2013 Science & Technology Review Evolutionary status of Zeta Orionis Aa+Ab CHARA/NPOI 2013 Science & Technology Review Sigma Orionis • AB = O9.5V + early BV, P = 157 yrs • Member of Sigma Ori cluster • Aa – Ab: 143 days • Ab: B0.5 V Simon-Diaz et al. 2011 Turner et al. 2008 CHARA/NPOI 2013 Science & Technology Review Tertiary component detected by NPOI Data from March 25, 2010 Turner et al. 2008 prediction Fit with improved orbit CHARA/NPOI 2013 Science & Technology Review Modifying Turner’s 2008 orbit CHARA/NPOI 2013 Science & Technology Review Sigma Orionis: close-pair orbit • a = 4.3 mas • e = 0.784 Peterson (priv. -
And Circumstellar Envelopes of Long Period Variable Stars
THE STRUCTURE OF HYDROXYL MASERS AND CIRCUMSTELLAR ENVELOPES OF LONG PERIOD VARIABLE STARS. Thesis by Mark Jonathan Reid In Partial Fulfillment of the Requirements For the degree of Doctor of Philosophy California Institute of Technology Pasadena, California 1975 (Submitted October 10, 1975) 1 Copyright © by Mark Jonathan Reid 1975 11 ACKNOWLEDGMENTS Throughout the two years it took to prepare this thesis, I have been helped by many people in a variety of ways. I wish to thank those people who have been so generous with their time, knowledge and effort on my behalf. To my wife, Katherine, I give special thanks for all the support and encouragement she has given me. Her influence and effort are evident throughout the text and in many of the drafted figures. I wi sh to thank my advisor, Duane Muhleman, for supporting the observing program when it seemed to be a lost cause, and for the almost daily assistance he has offered me during my four years of graduate work. The successful running of the VLB experiments was due to the efforts of many people. Duane Muhleman, James Moran, Kenneth Johnston, Phillip Schwartz, Jonathan Romney and Richard Schilizzi were very attentive during the actual observations. Jack Welch and the entire Hat Creek staff did an outstanding job keeping their telescope "on the air" almost every minute of the scheduled time. Peter and Holly Schloerb took a late night, impromptu "vacation" to the Owens Valley observatory to replace a broken video tape recorder and Harry Hardebeck lost that night's sleep modifying and adjusting the new recorder.