…These are cool, red, supergiants with large luminosity and radius, but their period is short and they evolve into main sequence stars in a fairly normal, stable state. However, stars with low mass go through a period of giant or subgiant starhood before the main sequence, and T Tauri stars are one of these. The majority of stars are main sequence stars, and are so named because they are distributed in a row on the Hertzsprung-Russell diagram (HR diagram) described below. … *Some of the terminology that mentions "subgiant stars" is listed below. Source | Heibonsha World Encyclopedia 2nd Edition | Information |
…これらは,温度が低く赤色で,光度も半径も大きい超巨星であるが,その時期は短くごくふつうの安定な状態にある主系列星へと進化する。ただし,質量のあまり大きくない星ではこの主系列前の巨星または亜巨星の時期があり,おうし座T型星はこれに相当する。恒星の大部分は主系列星であり,後出のヘルツシュプルング=ラッセル図(HR図)上に列をなして分布するのでこの名がある。… ※「亜巨星」について言及している用語解説の一部を掲載しています。 出典|株式会社平凡社世界大百科事典 第2版について | 情報 |
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