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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
一个不对称的冲击波在2006年爆发的反复新星RS Ophiuchichi的爆发
T J O'Brien1, M F Bode, R W Porcas
1Jodrell Bank Observatory, School of Physics & Astronomy, The University of Manchester, Macclesfield, Cheshire, SK11 9DL, UK. tim.obrien@manchester.ac.uk
Nature
|July 21, 2006
概括
像RS Ophiuchi这样的反复出现的新星会以喷射式的,而不是球形的爆发方式抛出物质. 这项研究揭示了RS Ophiuchi中膨胀的冲击波和协同抛射,类似于超新星残骸.
科学领域:
- 天体物理学 天体物理学
- 恒星进化 恒星进化
- X射线天文学X射线天文学
背景情况:
- 新星爆发是二进制星系中白矮星上的热核爆炸.
- 1985年RS Ophiuchi爆发的先前模型没有完全解释X射线数据或残留形态.
- 无线电观测表明双极残留物,与球形模型相矛盾.
研究的目的:
- 为了研究复发性新星RS Ophiuchi2006年爆发的残余的结构和演变.
- 为了解决关于残骸形状和弹射机制的争议.
- 为了确定中央二进制系统的方向.
主要方法:
- 在RS Ophiuchi中检测空间分辨结构,始于2006年爆发后两周.
- 通过红巨人的风追踪一个正在扩大的冲击波.
- 对非热 (同步子) 无线电辐射的分析.
主要成果:
- 观测到一个膨胀的冲击波创造了一个类似于II型超新星的残留物,但在几个月内演变.
- 无线电发射证实了非热同步子辐射.
- 不对称性和多重排放组件表明喷气式的,合并的喷射,而不是球形.
结论:
- 2006年RS Ophiuchi的爆发涉及喷气式喷射,这与之前的球形对称性假设相矛盾.
- 其余的结构提供了对中央二进制的聚合机制的见解.
- 通过观测,可以确定二进制系统的方向.
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