| 词条 | GQ Muscae |
| 释义 |
|constell= Musca |name= GQ Muscae |type= |ra= {{RA|11|52|02.35}} [1] |dec= {{DEC|-67|12|20.2}} [1] }}GQ Muscae, also known as Nova Muscae 1983 is a binary star system in the constellation Musca composed of a white dwarf and small star that is about 10% as massive as the Sun. The two orbit each other every 1.4 hours. The white dwarf accumulates material from its companion star on its accretion disc until it erupts, as it did in 1983, reaching a magnitude of 7.2.[2] Discovered with a magnitude of 7.1 on 18 January 1983,[3] it was the first nova from which X-rays were detected.[4] References1. ^1 {{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GQ+Mus&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id |title = NOVA Mus 1983 -- Nova |work = SIMBAD Astronomical Database|publisher=Centre de Données astronomiques de Strasbourg |accessdate = 9 March 2014}} {{Musca}}{{Var-star-stub}}2. ^{{cite journal|author1=Hachisu, Izumi |author2=Kato, Mariko |author3=Cassatella, Angelo |date=2008|title=A Universal Decline Law of Classical Novae. III. GQ Muscae 1983|journal=The Astrophysical Journal|volume=687|pages=1236–52|url=http://iopscience.iop.org/0004-637X/687/2/1236/fulltext/72628.text.html|bibcode=2008ApJ...687.1236H|arxiv = 0806.4253 |doi = 10.1086/591415 }} 3. ^{{cite book|last=Liller|first=William|title=Cambridge Astronomy Guide|publisher=CUP Archive|location=Cambridge, United Kingdom|date=1990|page=105|isbn=0-521-39915-7|url=https://books.google.com/books?id=yl04AAAAIAAJ&pg=PA105}} 4. ^{{cite journal|last=Duerbeck|first=H.W.|date=2009|title=New Stars and Telescopes: Nova Research in the Last Four Centuries|journal=Astronomische Nachrichten|volume=330|issue=6|pages=568–73|url=http://www.physics.usyd.edu.au/~laszlo/kepek/400ev_novai.pdf|doi=10.1002/asna.200911218|bibcode = 2009AN....330..568D }} 3 : Musca (constellation)|Objects with variable star designations|Novae |
| 随便看 |
|
开放百科全书收录14589846条英语、德语、日语等多语种百科知识，基本涵盖了大多数领域的百科知识，是一部内容自由、开放的电子版国际百科全书。