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HD 38282
HD 38282 (R144, BAT99-118, Brey 89) is a massive binary star in the Tarantula Nebula (Large Magellanic Cloud), consisting of two hydrogen-rich Wolf-Rayet stars.〔 Both stars are young and massive, amongst the most luminous known. They form a spectroscopic binary with a period of a few months. The orbit is not well known so the masses of the stars are only estimated. == See also ==
*List of most luminous 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「HD 38282」の詳細全文を読む
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