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Late-type star : ウィキペディア英語版 | Late-type star
In stellar classification, a late-type star is a star of class K or class M. The term was coined in the early 20th century, when there was a belief that stars began their history as early-type stars of class O, B, or A, and subsequently cooled to late-type stars.〔(late-type star ), David Darling, entry in ''The Internet Encyclopedia of Science''. Accessed on line October 14, 2007.〕 ==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「Late-type star」の詳細全文を読む
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