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星X-1包含一个21太阳质量的黑洞 - - 对巨大的恒星风的影响
James C A Miller-Jones1, Arash Bahramian2, Jerome A Orosz3
1International Centre for Radio Astronomy Research-Curtin University, Perth, WA 6845, Australia. james.miller-jones@curtin.edu.au.
概括
通过无线电天文测量, 精确了对黑洞二进制星体Cygnus X-1的距离. 这表明黑洞质量更高, 限制了巨大的恒星进化过程中的恒星风质量损失.
科学领域:
- 天体物理学
- 恒星进化
- 射线天文学
背景情况:
- 巨大的恒星进化受到恒星风的质量损失的影响.
- 恒星风会影响像黑洞这样的残余物体的最终质量.
- 精确的距离测量对于确定黑洞质量至关重要.
研究的目的:
- 为了精确距离黑洞X射线二进制天X-1.
- 为了确定Cygnus X-1黑洞的更精确的质量.
- 用这些发现来限制大质量恒星的质量损失模型.
主要方法:
- 使用无线电天文测量来测量位,从而测量到天X-1的距离.
- 结合新的距离测量与现有的存档光学数据.
- 根据轨道动态和精细的距离计算出黑洞的质量.
主要成果:
- 到Cygnus X-1的距离被确定为[FORMULA]千帕塞克.
- 黑洞的质量估计为21.2±2.2太阳质量,超过之前的估计.
- 这种在高金属度环境中的高质量挑战了当前的恒星进化模型.
结论:
- 星X-1黑洞的精细质量为恒星进化理论提供了关键数据.
- 这些发现表明恒星风可能从巨大的恒星中移除的质量比之前所认为的要少.
- 这项研究提供了对大质量恒星生命末期过程的新约束.
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