カーニナの大きな噴火
Kris Davidson1, Roberta M Humphreys
1Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA. kd@umn.edu
Nature
|June 23, 2012
まとめ
超新星インポスターイベントである巨大な恒星エタ・カリーナの大噴火は,新しい物理学を必要としないかもしれません. 新しい分析によると,観測されたスペクトルは,恒星物理学の既存の理論と一致している.
科学分野:
- 天文学と天体物理学について
- 恒星の進化について
- スーパーノワの詐欺師たち
背景:
- 巨大な恒星であるエタ・カリーナの1838-1858年の大噴火は,超新星インポスターイベントの重要な例です.
- このイベントは,超新星を模倣しながら,恒星を無傷のままにして,かなりの質量損失と明るさを含んでいた.
- 標準的な説明は,数年間にわたる過剰な放射線圧によって引き起こされた質量放出である.
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