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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク List of novae in the Milky Way galaxy ： ウィキペディア英語版 List of novae in the Milky Way galaxy This is a partial list of novae in the Milky Way galaxy that have been discovered and recorded since 1891. Novae are stars that undergo dramatic explosions, but unlike supernovae, these do not result in the destruction of the original star. The likely rate of novae in the Milky Way is about 40 per year,〔Prialnik, Dina. "Novae", pp. 1846-56, in Paul Murdin, ed. ''Encyclopedia of Astronomy and Astrophysics.'' London: Institute of Physics Publishing Ltd and Nature Publishing Group, 2001. ISBN 1-56159-268-4〕 but of these only about 10 per year are discovered by observers as of the 2000s (decade).〔(CBAT List of Novae in the Milky Way ) discovered since 1612〕 This list attempts to include only the brighter or more notable novae. The Central Bureau for Astronomical Telegrams (CBAT) maintains a more complete list of novae in the Milky Way since 1612.〔 ==Nomenclature== Novae are initially designated via a "Nova (form of constellation name ) (of discovery )" format, e.g. "Nova Cygni 1974" and "Nova Scorpii 2010". An official permanent name is usually soon assigned by the General Catalog of Variable Stars using the GCVS format for the naming of variable stars. When more than one nova is discovered in a constellation in one year, a numeric suffix is appended; hence "Nova Sagittarii 2011 #2", "Nova Sagitarii 2011 #3", etc. * Outburst in progress 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「List of novae in the Milky Way galaxy」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.