在一个孤立的年轻中子星周围的碎片盘
Zhongxiang Wang1, Deepto Chakrabarty, David L Kaplan
1Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.
Nature
|April 7, 2006
概括
天文学家在一个年轻的X射线脉冲星周围发现了一个冷盘,提供了超新星备用盘的证据. 这一发现表明,在中子星周围可能会形成行星.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 恒星进化 恒星进化
背景情况:
- 脉冲星是由超新星爆炸形成的旋转中子星.
- 超新星模型预测备用磁盘,但观测证据很少.
- 后备盘可能会影响脉冲星的演变和黑洞的形成.
研究的目的:
- 为了寻找脉冲星周围备用盘的观测证据.
- 为了研究一个X射线脉冲星周围新发现的磁盘的特性和起源.
主要方法:
- 从一个孤立的年轻X射线脉冲星观察到的中红外辐射.
- 分析了磁盘的属性,包括质量和寿命.
- 将磁盘特征与超新星回落的理论预测进行了比较.
主要成果:
- 在一个年轻的X射线脉冲星周围发现了一个凉爽的中红外发射盘.
- 磁盘的质量大约是地球的10个质量,其寿命超过106年.
- 该盘被脉冲星的X射线被动地照亮,类似于原行星盘.
结论:
- 观测到的磁盘支持超新星回落理论.
- 磁盘的属性与一个备用源相一致.
- 这一发现暗示了年轻中子星周围行星形成的可能性.
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