翻訳と辞書 Words near each other ・ VA-210 (U.S. Navy) ・ VA-212 (U.S. Navy) ・ V5 engine ・ V5 interface ・ V50 ・ V500 ・ V500 Aquilae ・ V509 Cassiopeiae ・ V518 Carinae ・ V520 Carinae ・ V529 Andromedae ・ V533 Carinae ・ V533 Herculis ・ V538 Aurigae ・ V539 Arae ・ V598 Puppis ・ V6 (band) ・ V6 (disambiguation) ・ V6 (Perl) ・ V6 (Quickstep) ・ V6 engine ・ V6 News ・ V60 ・ V602 Carinae ・ V603 Aquilae ・ V604 Aquilae ・ V605 Aquilae ・ V606 Aquilae ・ V636 Scorpii ・ V7 Dictionary Lists mini英和辞書 mini和英辞書 Webster 1913 Latin-English FOLDOC Wikipedia English ウィキペディア

翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク V598 Puppis ： ウィキペディア英語版 V598 Puppis V598 Puppis is the name given to a nova in the Milky Way Galaxy. USNO-A2.0 0450-03360039, the catalog number for the star, was discovered to be much brighter than normal in X-ray emissions on October 9, 2007, by the European Space Agency's XMM-Newton telescope.〔 〕 Ultimately, the star was confirmed to 600 times brighter than normal by the Magellan-Clay telescope Magellan-Clay telescope at Las Campanas Observatory in Chile. The nova has been officially named V598 Puppis and is "one of the brightest for almost a decade".〔 Despite its brightness, the nova was apparently missed by amateur and professional astronomers alike until XMM-Newton spotted the unusual X-ray source while turning from one target to another. The All Sky Automated Survey determined that that nova had occurred on June 5, 2007. ==References== 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「V598 Puppis」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.