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来自反复出现的新星RS Ophiuchichi的X射线发射的爆炸波
J L Sokoloski1, G J M Luna, K Mukai
1Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, Massachusetts 02138, USA. jsokoloski@cfa.harvard.edu
Nature
|July 21, 2006
概括
新星和超新星产生了重元素. 对反复出现的新星RS Ophiuchi的观测显示,其爆炸波迅速减速,表明它是一个低质量喷射物和高质量白矮星,一个潜在的Ia型超新星祖先.
科学领域:
- 天文学和天体物理学.
- 宇宙元素核合成的核合成
- 恒星进化中的恒星演变
背景情况:
- 像新星和超新星这样的恒星爆炸是重元素的主要来源.
- 新星的出现被理解为白矮星的表面热核逃跑,但喷射物质的特性仍然不清楚.
- 星云中的反复出现的新星为爆炸动态和元素分布提供了独特的见解.
研究的目的:
- 为了研究在爆发期间反复出现的新星RS Ophiuchi的X射线发射和冲击波动力学.
- 为了确定喷射物和白矮星的质量和结构.
- 评估对Ia型超新星的祖先的影响.
主要方法:
- 利用X射线观测来研究反复出现的新星RS Ophiuchi的爆发.
- 分析了来自爆炸波背后的硬X射线辐射.
- 研究了冲击波与周围星云相互作用的膨胀和减速.
主要成果:
- 在喷发的早期阶段,观察到从爆炸波背后发出的硬X射线辐射.
- 爆炸波在不到2天的时间内自由扩张,然后由于星云相互作用而减速.
- 快速色的X射线表明偏离标准的球形外结构,并表明射物质较低,白矮星质量较高.
结论:
- RS Ophiuchi的快速减速意味着喷射物质很低,而白矮星的质量很高.
- 该系统是Ia型超新星的潜在祖先,对于理解宇宙膨胀至关重要.
- 这些发现完善了新星爆炸的模型及其对银河系化学进化的贡献.
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