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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 Messier 90 ： ウィキペディア英語版 Messier 90 Messier 90 (also known as ''M90'' and ''NGC 4569'') is a spiral galaxy about 60 million light-years away in the constellation Virgo. It was discovered by Charles Messier in 1781.〔 〕 == Membership of the Virgo Cluster == Messier 90 is a member of the Virgo Cluster.〔 〕 and one of its largest and brightest spiral galaxies, with an absolute magnitude of around -22 (brighter than the Andromeda Galaxy).〔 The galaxy is located approximately 1°.5 away from the subgroup centered on Messier 87.〔 〕 As a consequence of the galaxy's interaction with the intracluster medium in the Virgo Cluster, the galaxy has lost much of its interstellar medium. As a result of this process, which is referred to as ''ram-pressure stripping'', the galaxy's interstellar medium and star formation regions appear severely truncated compared to similar galaxies outside the Virgo Cluster〔 〕 and there're even H II regions outside the galactic plane.〔 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「Messier 90」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.