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Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
Published on: May 10, 2020
超新星爆炸中的无球性来自于晚期光谱学的超新星爆炸
Keiichi Maeda1, Koji Kawabata, Paolo A Mazzali
1Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, Kashiwa-no-ha 5-1-5, Kashiwa City, Chiba 277-8582, Japan. maeda@ea.c.u-tokyo.ac.jp
概括
大多数来自剥离外恒星的核心崩超新星 (CC-SNe) 都显示出不对称爆炸的迹象. 与玛射线爆发 (GRBs) 相关的显示最显著的不对称性.
科学领域:
- 天体物理学 天体物理学
- 恒星进化 恒星进化
- 超新星是指一个超新星.
背景情况:
- 核心崩超新星 (CC-SNe) 标志着大质量恒星生命的结束.
- 一些CC-SNe与高度不对称的,长时间的马射线爆发 (GRB) 有关.
- 在所有CC-SNe中不对称的普遍性仍然是一个开放的问题.
研究的目的:
- 为了调查剥离包裹CC-SNe.内在区域的asphericity的程度.
- 为了确定非对称性是否是所有CC-SNe从剥离封面恒星的共同特征.
主要方法:
- 分析多个CC-SNe来自剥离包膜恒星的晚期光谱.
- 对氧气排放线形状的检查,以寻找不对称爆炸的特征.
- 与GRB相关的超新星和其他CC-SNe.之间的不对称水平的比较.
主要成果:
- 观察到的CC-SNe的很大一部分呈现出双峰氧气排放线.
- 这些双峰形状标志着爆炸的非对称喷射物.
- 这项研究发现,从剥离封面恒星中,CC-SNe中存在高频率的不对称性.
结论:
- 所有来自剥离外恒星的核心崩超新星似乎都是不对称的爆炸.
- 与马射线爆发相关的超新星表现出最高度的无球性.
- 非对称性是剥离外超新星的基本特征,GRB相关事件是最极端的.
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