Jrasc#4 2001 Outside Cover
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Sirius Astronomer Newsletter
March 2004 Free to members, subscriptions $12 for 12 issues Volume 31, Number 3 Images completed in 2002 (left) and 2003 (right) depict the analemma. The analemma illustrates the motion of the sun across the sky when observed from precisely the same place and precisely the same time of the day over the course of a year. The ruins in the 2002 photo are those of Tholos, ancient Delphi, Greece; the ruins in the 2003 photo are those of the Temple of Zeus, ancient Nemea, Greece. For more information, see http://www.perseus.gr/Astro-Solar-Analemma.htm (courtesy Anthony Ayiomamitis). OCA CLUB MEETING STAR PARTIES COMING UP The free and open club The Black Star Canyon site will be open this The next session of the meeting will be held Friday, month on March 13th. The Anza site will be Beginners Class will be held on March 12th at 7:30 PM in open March 20th. Members are encouraged Friday March 5th (and next the Irvine Lecture Hall of the to check the website calendar, for the latest month on April 2nd) at the Hashinger Science Center updates on star parties and other events. Centennial Heritage Museum at Chapman University in (formerly the Discovery Museum Orange. The featured Please check the website calendar for the of Orange County) at 3101 speaker this month is Luisa outreach events this month! Volunteers West Harvard Street in Santa Rebull, who will tell us are always welcome! Ana. “What’s New With SIRTF”. You are also reminded to check the web GOTO SIG: TBA (contact NOTE: The April Meeting site frequently for updates to the calendar coordinator for details) has been rescheduled to of events and other club news. -
LIST of PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute
LIST OF PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute of Department of Science and Technology, Govt. of India) Manora Peak, Naini Tal - 263 129, India (1955−2020) ABBREVIATIONS AA: Astronomy and Astrophysics AASS: Astronomy and Astrophysics Supplement Series ACTA: Acta Astronomica AJ: Astronomical Journal ANG: Annals de Geophysique Ap. J.: Astrophysical Journal ASP: Astronomical Society of Pacific ASR: Advances in Space Research ASS: Astrophysics and Space Science AE: Atmospheric Environment ASL: Atmospheric Science Letters BA: Baltic Astronomy BAC: Bulletin Astronomical Institute of Czechoslovakia BASI: Bulletin of the Astronomical Society of India BIVS: Bulletin of the Indian Vacuum Society BNIS: Bulletin of National Institute of Sciences CJAA: Chinese Journal of Astronomy and Astrophysics CS: Current Science EPS: Earth Planets Space GRL : Geophysical Research Letters IAU: International Astronomical Union IBVS: Information Bulletin on Variable Stars IJHS: Indian Journal of History of Science IJPAP: Indian Journal of Pure and Applied Physics IJRSP: Indian Journal of Radio and Space Physics INSA: Indian National Science Academy JAA: Journal of Astrophysics and Astronomy JAMC: Journal of Applied Meterology and Climatology JATP: Journal of Atmospheric and Terrestrial Physics JBAA: Journal of British Astronomical Association JCAP: Journal of Cosmology and Astroparticle Physics JESS : Jr. of Earth System Science JGR : Journal of Geophysical Research JIGR: Journal of Indian -
Übersicht NGC-Objektauswahl Cepheus Zur Übersichtskarte
NGC-Objektauswahl Cepheus NGC 40 NGC 7055 NGC 7354 NGC 188 NGC 7076 NGC 7380 NGC 1184 NGC 7129 NGC 7419 NGC 1544 NGC 7139 NGC 7423 NGC 2276 NGC 7142 NGC 7429 NGC 2300 NGC 7160 NGC 7510 NGC 6939 NGC 7226 NGC 7538 NGC 6949 NGC 7235 NGC 7708 NGC 6951 NGC 7261 NGC 7762 NGC 7023 NGC 7281 NGC 7822 Sternbild- Übersicht Zur Objektauswahl: Nummer anklicken Zur Übersichtskarte: Objekt anklicken Sternbildübersicht Auswahl NGC 40_7708 Aufsuchkarte Auswahl NGC 188_Aufsuchkarte 2 UMi 2 Auswahl NGC 1184 Aufsuchkarte Auswahl NGC 1544_2276_2300 Aufsuchkarte Auswahl NGC 6939 Aufsuchkarte Auswahl NGC 6949_6951 Aufsuchkarte Auswahl NGC 7023 Aufsuchkarte Auswahl NGC 7055 Aufsuchkarte Auswahl NGC 7076 Aufsuchkarte Auswahl NGC 7129_7142 Aufsuchkarte Auswahl NGC 7139_7160 Aufsuchkarte Auswahl NGC 7226_7235 Aufsuchkarte Auswahl N 7261_7281 Aufsuchkarte Auswahl NGC 7354_7419_7429_7510_7538 Aufsuchkarte Auswahl NGC 7380_7423 Aufsuchkarte Auswahl NGC 7762_7822 Aufsuchkarte Auswahl NGC 40 Übersichtskarte Aufsuch- Auswahl karte NGC 188 Übersichtskarte Aufsuch- Auswahl karte NGC 1184 Übersichtskarte Aufsuch- Auswahl karte NGC 1544 Übersichtskarte Aufsuch- Auswahl karte N 2276_N 2300 Übersichtskarte Aufsuch- Auswahl karte NGC 6939 Übersichtskarte Aufsuch- Auswahl karte NGC 6949 Übersichtskarte Aufsuch- Auswahl karte NGC 6951 Übersichtskarte Aufsuch- Auswahl karte NGC 7023 Übersichtskarte Aufsuch- Auswahl karte NGC 7055 Übersichtskarte Aufsuch- Auswahl karte NGC 7076 Übersichtskarte Aufsuch- Auswahl karte NGC 7129_7142 Übersichtskarte Aufsuch- Auswahl karte NGC 7139 -
A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair
ASTRONOMY AND ASTROPHYSICS - A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair A HISTORY OF ASTRONOMY, ASTROPHYSICS AND COSMOLOGY Malcolm Longair Cavendish Laboratory, University of Cambridge, JJ Thomson Avenue, Cambridge CB3 0HE Keywords: History, Astronomy, Astrophysics, Cosmology, Telescopes, Astronomical Technology, Electromagnetic Spectrum, Ancient Astronomy, Copernican Revolution, Stars and Stellar Evolution, Interstellar Medium, Galaxies, Clusters of Galaxies, Large- scale Structure of the Universe, Active Galaxies, General Relativity, Black Holes, Classical Cosmology, Cosmological Models, Cosmological Evolution, Origin of Galaxies, Very Early Universe Contents 1. Introduction 2. Prehistoric, Ancient and Mediaeval Astronomy up to the Time of Copernicus 3. The Copernican, Galilean and Newtonian Revolutions 4. From Astronomy to Astrophysics – the Development of Astronomical Techniques in the 19th Century 5. The Classification of the Stars – the Harvard Spectral Sequence 6. Stellar Structure and Evolution to 1939 7. The Galaxy and the Nature of the Spiral Nebulae 8. The Origins of Astrophysical Cosmology – Einstein, Friedman, Hubble, Lemaître, Eddington 9. The Opening Up of the Electromagnetic Spectrum and the New Astronomies 10. Stellar Evolution after 1945 11. The Interstellar Medium 12. Galaxies, Clusters Of Galaxies and the Large Scale Structure of the Universe 13. Active Galaxies, General Relativity and Black Holes 14. Classical Cosmology since 1945 15. The Evolution of Galaxies and Active Galaxies with Cosmic Epoch 16. The Origin of Galaxies and the Large-Scale Structure of The Universe 17. The VeryUNESCO Early Universe – EOLSS Acknowledgements Glossary Bibliography Biographical SketchSAMPLE CHAPTERS Summary This chapter describes the history of the development of astronomy, astrophysics and cosmology from the earliest times to the first decade of the 21st century. -
Journal Für Astronomie ISSN 1615-0880
Journal für Astronomie www.vds-astro.de ISSN 1615-0880 Nr. 75 4/2020 Zeitschrift der Vereinigung der Sternfreunde e.V. Infrarotastronomie ASTRONOMISCHE VEREINIGUNGEN Die Sternwarte St. Andreasberg KOMETEN Die Entwicklung von C/2020 F3 (NEOWISE) PLANETEN Die Sichtbarkeit von Venus im Frühjahr 2020 Canon EOS 250D & 2000D modifiziert für die Astrofotografie ! Ob mit Kameraobjektiv oder am Teleskop: Modizierte Canon EOS DSLR Kameras bieten Ihnen einen einfachen Einstieg in die Astrofotograe! Die Vorteile im Überblick: • etwa fünffach höhere Empfindlichkeit bei H-alpha und SII • Infrarot Blockung der Kamera bleibt vollständig erhalten • kein Einbau eines teuren Ersatzfilters • mit Astronomik OWB-Clip-Filter uneingeschränkt bei Tag nutzbar • auch ohne Computer am Teleskop einsatzfähig • 14 Bit Datentiefe im RAW-Format, 24 Megapixel • bei der 250Da: Erhalt des EOS Integrated Cleaning System • bei der 250Da: Dreh- und schwenkbarer Bildschirm • kompatibel mit vielen gängigen Astronomieprogrammen • voller Erhalt der Herstellergarantie Weitere Modelle auf Anfrage Wir bauen auch Ihre bereits vorhandene Kamera um! Canon EOS 250Da € 72037 * Canon EOS 2000Da € 54491 * * Tagespreis vom 07. August 2020 mit 200mm 1:4 Reflektor ©Bruno Mattern, Aufnahme Astronomik Deep-Sky RGB Farbfiltersatz Neuentwicklung! + optimierte Bildschärfe + höchster Kontrast + maximale Transmission = optimale Ergebnisse © Michael Sidonio Annals of the Deep Sky - A Survey of Galactic and Extragalactic Objects astro-shop Diese englischsprachige Buchreihe ist als mehrbändiges Werk angelegt, das Das seit zwei Jahrzehnten erfolgreiche Konzept die heutige Sicht auf alle Sternbilder des Himmels und die in Ihnen beobacht- hat inzwischen viele Nachahmer gefunden. baren Objekte darstellt. Deshalb achten Sie unbedingt darauf, dass Sie Die Gliederung erfolgt alphabetisch nach Sternbildern. Vergleichbar sind die auf der richtigen astro-shop Seite landen: Bücher mit "Burnham's Celestial Handbook" oder "Taschenatlas der Sternbilder“, eben aktualisiert auf den Wissens- und Technikstand von heute. -
Curriculum Vitæ
Curriculum vitæ Robert Andrew Ernest Fosbury as of: June 2012 Date of birth: 2nd April 1948 Place: Farnham, Surrey, England Nationality: British Present address: Michael-Huber-Weg 12 81667 München Germany Tel:+49 89 609 96 50 [domiciled in Germany] Email: [email protected] ; [email protected] Married to: Patricia Susan Fosbury (née Major-Allen) Children: Emma Louise – 1974, England Thomas Benjamin – 1977, Australia Andrew Daniel – 1977, Australia Present employer: European Southern Observatory Karl Schwarzschild Straße 2 85748 Garching bei München Germany Tel: +49 89 320 06 235 Societies: Fellow of the Royal Astronomical Society, Council service 1983, 1984 Member of the International Astronomical Union Fluorescent Mineral Society: member of Research Chapter Present job 2011–> European Southern Observatory (ESO) Astronomer Emeritus. I am also employed part-time by ESO to perform certain functions for them including editing the ESO Annual Report (http://www.eso.org/public/products/annualreports/ann-report2010/ ) and representing ESO (as an observer) at the United Nations Committee on the Peaceful Uses of Outer Space. As part of this UN work, I am a member of Action Team 14 which is tasked to make recommendations to the General Assembly and the Security Council for the mitigation of the threat of Earth impact of potentially hazardous Near Earth Asteroids (NEO). Also, I currently serve on the European Research Council panel for the evaluation of Advanced Grant proposals in Universe Sciences. Previous jobs and appointments 2003–2006 Visiting Professor at the University of Sheffield 1985–2010 Staff member (ESA) of the (Hubble) Space Telescope – European Coordinating Facility (ST-ECF): co-funded by the European Space Agency (ESA) and the European Southern Observatory and hosted by the latter organization at its headquarters near Munich. -
Astronomy 142 — Project Manual Spring 2021
Astronomy 142 | Project Manual Spring 2021 1 RR Lyrae stars and the distance to globular cluster M3 1.1 Introduction In the following, we repeat a classic experiment: detect the periodically-varying stars in a globular cluster and thereby measure its distance, by considering the stars to be standard candles. Specifi- cally, we will measure the time-average luminosity of the nearby star RR Lyrae and the time-average flux of stars in M3 that vary with the same period as RR Lyr, combining these measurements to determine M3's distance. This observing project will involve frequent remote observation sessions with the tele- scope over the course of 1{2 weeks, hopefully including a few nights in a row. Everyone who opts for this project will share their data and receive everyone else's in return. Each student will perform his or her own analysis and write an independent report on the results. Stars in the instability strip of the HR diagram have been fundamental in the determination of the distance scale of the Universe. These stars radially pulsate, often in their fundamental acoustic mode. As we have seen in class, their pulsation periods Π vary inversely with the mass density ρ of the star: Z R dr r 6π Π = 4 =∼ (uniform density star) (1) 0 vs γGρ Lower average density leads not only to longer periods, but also to larger luminosities L, in part because lower-density stars are much larger than higher-density stars of the same mass. Thus, a given type of pulsating star exhibits a strict relation, often linear, between Π and L. -
Table of Contents
AAS Newsletter July/August 2011, Issue 159 - The Online Publication for the members of the American Astronomical Society Table of Contents President's Column 2 2011 Chrétien Grant Winner 11 From the Executive Office 4 IAU Membership Deadline 11 Secretary's Corner 5 Highlights from the Hub of the Council Actions 6 Universe 12 Journals Update 8 SPD Meeting 23 25 Things About... 9 Washington News Back Page A A S American Astronomical Society AAS Officers President's Column Debra M. Elmegreen, President David J. Helfand, President-Elect Debra Meloy Elmegreen, [email protected] Lee Anne Willson, Vice-President Nicholas B. Suntzeff, Vice-President Edward B. Churchwell, Vice-President Hervey (Peter) Stockman, Treasurer G. Fritz Benedict, Secretary Richard F. Green, Publications Board Chair We hit a homerun in Boston with Timothy F. Slater, Education Officer one of our biggest summer meetings Councilors ever, including over 1300 registrants; Bruce Balick still, it had the more intimate feel that Richard G. French Eileen D. Friel characterizes our summer gatherings. It Edward F. Guinan was a privilege to share our 218th meeting Patricia Knezek James D. Lowenthal with the American Association of Robert Mathieu Variable Star Observers on the occasion Angela Speck th Jennifer Wiseman of their 100 anniversary, and to present them a certificate to commemorate Executive Office Staff the long-time professional-amateur Kevin B. Marvel, Executive Officer Tracy Beale, Membership Services collaboration we have all enjoyed. Administrator Margaret Geller gave a stirring Henry Chris Biemesderfer, Director of Publishing Laronda Boyce, Meetings & Exhibits Norris Russell Lecture on her discovery Coordinator of large-scale structure in the Universe. -
A Selection of New Arrivals September 2017
A selection of new arrivals September 2017 Rare and important books & manuscripts in science and medicine, by Christian Westergaard. Flæsketorvet 68 – 1711 København V – Denmark Cell: (+45)27628014 www.sophiararebooks.com AMPERE, Andre-Marie. Mémoire. INSCRIBED BY AMPÈRE TO FARADAY AMPÈRE, André-Marie. Mémoire sur l’action mutuelle d’un conducteur voltaïque et d’un aimant. Offprint from Nouveaux Mémoires de l’Académie royale des sciences et belles-lettres de Bruxelles, tome IV, 1827. Bound with 18 other pamphlets (listed below). [Colophon:] Brussels: Hayez, Imprimeur de l’Académie Royale, 1827. $38,000 4to (265 x 205 mm). Contemporary quarter-cloth and plain boards (very worn and broken, with most of the spine missing), entirely unrestored. Preserved in a custom cloth box. First edition of the very rare offprint, with the most desirable imaginable provenance: this copy is inscribed by Ampère to Michael Faraday. It thus links the two great founders of electromagnetism, following its discovery by Hans Christian Oersted (1777-1851) in April 1820. The discovery by Ampère (1775-1836), late in the same year, of the force acting between current-carrying conductors was followed a year later by Faraday’s (1791-1867) first great discovery, that of electromagnetic rotation, the first conversion of electrical into mechanical energy. This development was a challenge to Ampère’s mathematically formulated explanation of electromagnetism as a manifestation of currents of electrical fluids surrounding ‘electrodynamic’ molecules; indeed, Faraday directly criticised Ampère’s theory, preferring his own explanation in terms of ‘lines of force’ (which had to wait for James Clerk Maxwell (1831-79) for a precise mathematical formulation). -
Making a Sky Atlas
Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it. -
Herschel II Lista Di Herschel II
Herschel II Lista di Herschel II Oltre i 400 Pagina 1 Gabriele Franzo Herschel II Chart R.A. Dec. Size Size Object OTHER Type Con. Mag. SUBR Class NGC Description No. ( h m ) ( o ' ) max min 61 NGC 23 UGC 89 GALXY PEG 00 09.9 +25 55 12 13 2.5 m 1.6 m SBa 3 S st + neb 109 NGC 24 ESO 472-16 GALXY SCL 00 09.9 -24 58 11,6 13,7 6.1 m 1.4 m Sc vF,cL,mE,gbm 85 NGC 125 UGC 286 GALXY PSC 00 28.8 +02 50 12,1 13 1.8 m 1.6 m Sa Ring vF,S,bM,D * sp 85 NGC 151 NGC 153 GALXY CET 00 34.0 -09 42 11,6 13,4 3.8 m 1.6 m SBbc pF,pL,lE 90 degrees,vglbM 109 NGC 175 NGC 171 GALXY CET 00 37.4 -19 56 12,2 13,5 2.1 m 1.9 m SBab pB,pL,E,gbM,r 85 NGC 198 UGC 414 GALXY PSC 00 39.4 +02 48 13,1 13,4 1.1 m 1.1 m Sc F,S,vgbM 37 NGC 206 G+C+N AND 00 40.5 +40 44 99,9 99,9 Pec vF,vL,mE 0 degrees 61 NGC 214 UGC 438 GALXY AND 00 41.5 +25 30 12,3 13,1 1.9 m 1.5 m SBc pF,pS,gvlbM,R 85 NGC 217 MCG - 2- 2- 85 GALXY CET 00 41.6 -10 01 13.5p 99,9 2.7 m 0.6 m Sa F,S,lE 90 degrees,glbM 61 NGC 315 UGC 597 GALXY PSC 00 57.8 +30 21 11,2 13,2 3 m 2.5 m E-SO pB,pL,R,gbM,* 9 nf 3' 85 NGC 337 MCG - 1- 3- 53 GALXY CET 00 59.8 -07 35 11,6 13,3 3 m 1.8 m SBcd pF,L,E,glbM,* 10 f 21 sec 84 NGC 357 MCG - 1- 3- 81 GALXY CET 01 03.4 -06 20 12 13,4 2.5 m 1.7 m SBO-a F,S,iR,sbM,* 14 nf 20'' 60 NGC 410 UGC 735 GALXY PSC 01 11.0 +33 09 11,5 12,7 2.3 m 1.8 m SB0 pB,pL,nf of 2 84 NGC 428 UGC 763 GALXY CET 01 12.9 +00 59 11,5 14,1 4 m 2.9 m Scp F,L,R,bM,er 60 NGC 499 IC 1686 GALXY PSC 01 23.2 +33 28 12,1 12,8 1.7 m 1.3 m E-SO pB,pL,R,3rd of 3 60 NGC 513 UGC 953 GALXY AND 01 24.4 +33 48 12,9 11,1 0.7 m -
Discrepancies in the Ages of Young Star Clusters; Evidence for Mergers?
MNRAS 000, 1–9 (2015) Preprint 14 March 2019 Compiled using MNRAS LATEX style file v3.0 Discrepancies in the ages of young star clusters; evidence for mergers? Emma R. Beasor1⋆, Ben Davies1, Nathan Smith2 and Nate Bastian1 1Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK 2Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA Accepted XXX. Received YYY; in original form ZZZ ABSTRACT There is growing evidence that star clusters can no longer be considered simple stellar populations (SSPs). Intermediate and old age clusters are often found to have ex- tended main sequence turn-offs (eMSTOs) which are difficult to explain with single age isochrones, an effect attributed to rotation. In this paper, we provide the first characterisation of this effect in young (<20Myr) clusters. We determine ages for 4 young massive clusters (2 LMC, 2 Galactic) by three different methods: using the brightest single turn-off (TO) star; using the luminosity function (LF) of the TO; and by using the lowest Lbol red supergiant (RSG). The age found using the cluster TO is consistently younger than the age found using the lowest RSG Lbol. Under the assump- tion that the lowest luminosity RSG age is the ‘true’ age, we argue that the eMSTOs of these clusters cannot be explained solely by rotation or unresolved binaries. We speculate that the most luminous stars above the TO are massive blue straggler stars formed via binary interaction, either as mass gainers or merger products. Therefore, using the cluster TO method to infer ages and initial masses of post-main sequence stars such as Wolf-Rayet stars, luminous blue variables and RSGs, will result in ages inferred being too young and masses too high.