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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 VFTS 682 ： ウィキペディア英語版 VFTS 682 VFTS 682 is a Wolf–Rayet star in the Large Magellanic Cloud. It is located over north-east of the massive cluster R136 in the Tarantula Nebula.〔 It is 150 times the mass of the sun and 3.2 million times more luminous which makes it one of the most massive and most luminous stars known. ==Discovery== VFTS 682 is a prominent infrared source in the Large Magellanic Cloud and has been catalogued numerous times. In 1992 it was identified as entry 153 in a list of possible protostars. In 2009 it was again classified as a probable young stellar object on account of its exceptional infrared luminosity. The VLT-FLAMES Tarantula survey (VFTS) examined 800 massive stars in detail and determined a spectral type of WN5h for VFTS 682. It is heavily reddened and visually several magnitudes fainter than other stars of similar luminosity and temperature in the 30 Doradus region.〔 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「VFTS 682」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.