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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 Hubble–Reynolds law ： ウィキペディア英語版 Hubble–Reynolds law The Hubble–Reynolds law models the surface brightness of elliptical galaxies as :$I(R)\; =\; \backslash frac$ Where $I(R)$ is the surface brightness at radius $R$, $I\_0$ is the central brightness, and $R\_H$ is the radius at which the surface brightness is diminished by a factor of 1/4. It is asymptotically similar to the De Vaucouleurs' law which is a special case of the Sersic profile for elliptical galaxies.〔Binney & Tremaine. ''Galactic Dynamics'' 2008.〕 The law is named for the astronomers Edwin Hubble and John Henry Reynolds. ==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「Hubble–Reynolds law」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.