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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 Rubin–Ford effect ： ウィキペディア英語版 Rubin–Ford effect The Rubin–Ford effect is the observation of a dipole anisotropy in the recessional velocity of a sample of ScI galaxies. This anisotropy is different in magnitude and direction from that of the cosmic microwave background radiation, and suggests that they are moving relative to the microwave background frame at about 800 km/s in the direction of the constellation Pegasus. It was found in 1976 by Vera Rubin and W. Kent Ford and became the subject of much discussion and interpretation over the following years. ==References== * Rubin, Ford, Thonnard, Roberts & Graham. "Motion of the Galaxy and the local group determined from the velocity anisotropy of distant SC I galaxies." 1976. Astronomical Journal, vol 81 pp 687–737 () (). 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「Rubin–Ford effect」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.