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超大質量恒星である30 doradus星雲の中央物体である

J P Cassinelli, J S Mathis, B D Savage

    Science (New York, N.Y.)
    |June 26, 1981
    PubMed
    まとめ

    30 Doradus Nebulaの構成要素であるR136aは,極端な性質を示し,それはクラスターではなく,単一の超光る星である可能性を示唆しています. この天体は,巨大な恒星風と星雲のイオン化を引き起こしています.

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