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从恒星风的光谱观测中得出的SN 2013cu的狼-雷耶特样的祖先
Avishay Gal-Yam1, I Arcavi1, E O Ofek1
1Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel.
Nature
|May 23, 2014
概括
大规模的狼-雷耶恒星可能会作为超新星爆炸. 我们在超新星2013cu中检测到沃尔夫-雷耶特风信号,这表明WN(h) 的祖先和爆炸前的质量损失.
科学领域:
- 恒星天体物理学 恒星天体物理学
- 超新星物理学 超新星物理学
背景情况:
- 大型狼-雷耶恒星 (WRSs) 是缺乏的超新星的潜在祖先.
- 之前的祖先鉴定是不确定的,或者导致没有检测.
研究的目的:
- 为了确定超新星2013cu (IIb型超新星) 的祖先.
- 为了研究超新星光谱中的狼-雷耶特式风信号.
主要方法:
- 闪光光谱学被用来捕捉2013cu. 的超新星冲击突破光谱.
- 分析的重点是确定指示恒星风的排放线.
主要成果:
- 在2013cu频谱中检测到与沃尔夫-雷耶特风标签一致的强排放线.
- 这些签名表明它是狼雷耶恒星WN(h) 亚类的祖先.
- 密集的风可能表明爆炸前质量损失增加.
结论:
- 2013cu超新星的祖先很可能是WN(h) 子类的缺水狼雷耶星.
- 这一发现支持了将沃尔夫-雷耶星与缺乏的超新星联系起来的理论.
- 这些结果与理论预测一致,即在恒星爆炸之前,质量损失会增加.
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