玛射线爆发的祖先恒星的属性
Pawan Kumar1, Ramesh Narayan, Jarrett L Johnson
1Astronomy Department, University of Texas, Austin, TX 78712, USA. pk@astro.as.utexas.edu
概括
研究人员估计了产生马射线爆发的恒星的物理特性. 该研究发现恒星核心半径为 (1-3) x10^10厘米,外半径为 (1-2) x10^11厘米,密度简介浅.
科学领域:
- 天体物理学 天体物理学
- 恒星进化 恒星进化
背景情况:
- 马射线爆发 (GRBs) 是强大的宇宙爆炸.
- 了解GRB的祖先恒星对于天体物理学至关重要.
研究的目的:
- 确定导致马射线爆发的恒星的基本物理性质.
- 调查GRB中快速发射和平原阶段背后的机制.
主要方法:
- 利用了三次GRB事件的X射线数据.
- 应用黑洞积聚和恒星结构的模型.
主要成果:
- 估计的恒星核心半径: (1-3) x 10^10厘米.
- 估计的恒星外半径: (1-2) x 10^11厘米.
- 在恒星外中确定了一个浅密度配置 (ρ r^-2).
- 计算出核心和外旋转速度大约分别为凯普勒速度的0.05和0.2.
结论:
- 积到一个中央黑洞可能会导致GRB发射.
- 恒星外的回落和积累解释了X射线高原阶段.
- 由此衍生的恒星属性为GRB祖先模型提供了约束.
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