翻訳と辞書 Words near each other ・ Gammertingen ・ Gammleng Award ・ Gammoid ・ Gammon ・ Gamma Strike ・ Gamma subunit ・ Gamma Tauri ・ Gamma test ・ Gamma Theta Phi ・ Gamma Theta Upsilon ・ Gamma Trianguli ・ Gamma Trianguli Australis ・ Gamma Tucanae ・ Gamma Ursae Majoris ・ Gamma Ursae Minoris ・ Gamma Velorum ・ Gamma Virginis ・ Gamma Volantis ・ Gamma wave ・ Gamma World ・ Gamma Zeta Alpha ・ Gamma-150 RNA motif ・ Gamma-Amanitin ・ Gamma-Amino-beta-hydroxybutyric acid ・ Gamma-aminobutyrate aminotransaminase ・ Gamma-aminobutyrate transaminase ・ Gamma-Aminobutyric acid ・ Gamma-aminobutyric acid aminotransferase ・ Gamma-aminobutyric acid receptor subunit alpha-1 ・ Gamma-aminobutyric transaminase 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 Gamma Velorum ： ウィキペディア英語版 Gamma Velorum }} Gamma Velorum (γ Vel, γ Velorum) is a multiple star system in the constellation Vela. At magnitude +1.7, it is one of the brightest stars in the night sky, and by far the closest and brightest Wolf-Rayet star. It has the traditional names Suhail and Suhail al Muhlif, which confusingly also apply to Lambda Velorum. It also has a more modern popular name Regor. ==Distance== Gamma Velorum is close enough to have accurate parallax measurements as well as distance estimates by more indirect means. The Hipparcos parallax for γ2 implies a distance of 342 pc. A dynamical parallax derived from calculations of the orbital parameters gives a value of 336 pc, similar to spectrophotometric derivations. A VLTI interferometry measurement of the distance gives a slightly larger value of 368 pc. All these distances are somewhat less than the commonly assumed distance of 450 pc for the Vela OB2 association which is the closest grouping of young massive stars. 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「Gamma Velorum」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.