一个超发光的X射线源由一个积聚中子星提供动力
M Bachetti1, F A Harrison2, D J Walton2
11] Université de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planétologie, 9, Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France [2] CNRS, Institut de Recherche en Astrophysique et Planétologie, 9, Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France.
Nature
|October 10, 2014
概括
超发光的X射线源,通常被认为是黑洞,可以是磁性中子星. 这些发现挑战了当前对紧物体积累的模型.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- X射线天文学X射线天文学
背景情况:
- 超发光X射线源 (ULX) 通常超过恒星质量黑洞的爱丁顿极限.
- 由于质量要求,理论模型偏好ULX的黑洞系统.
- 解释最明亮的ULXs (> 10^40 ergs/sec) 需要巨大的黑洞或非标准的积累.
研究的目的:
- 为了研究超发光X射线源的性质.
- 确定中子星是否可以为ULXs的种群做出贡献.
- 挑战和完善现有的积累物理模型.
主要方法:
- 对M82星系核区域的宽带X射线观测.
- 对X射线发射中的脉冲和侧侧模拟的分析.
- 脉动和可变X射线源的空间巧合分析.
主要成果:
- 从M82.82的源头发现脉冲 (1.37s周期) 和二进制调制 (2.5d周期).
- 脉冲流表示光度为4.9 × 10^39 ergs/秒 (3-30 keV).
- 该源达到1.8 × 10^40 ergs/sec (0.3-10 keV),大约是1.4太阳质量中子星的埃丁顿极限的100倍.
结论:
- 磁性中子星可以是超发光的X射线源.
- 这一发现挑战了ULX仅仅是黑洞系统的假设.
- 观测到的亮度表明中子星可能在ULX中很常见,并推动了积累模型的界限.
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