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Hyperpolarized Xenon for NMR and MRI Applications
Published on: September 6, 2012
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由两种类型的超新星产生的两种X射线脉冲星群
Christian Knigge1, Malcolm J Coe, Philipp Podsiadlowski
1University of Southampton, School of Physics and Astronomy, Southampton SO17 1BJ, UK. c.knigge@soton.ac.uk
Nature
|November 15, 2011
概括
科学家在Be/X射线双星类中发现了两个不同的中子星群,它们可能来自不同的超新星类型. 电子捕获超新星似乎形成中子星,旋转和轨道周期较短,离心率较低.
科学领域:
- 天体物理学 天体物理学
- 恒星进化 恒星进化
- 中子星形成的过程
背景情况:
- 中子星主要是通过铁核崩超新星和电子捕获超新星形成的.
- 由这两个不同的形成通道产生的中子星之间的区别一直是具有挑战性的.
- 射线/X射线双星,X射线脉冲星的一类,宿主中子星从伴星中积聚.
研究的目的:
- 调查Be/X射线二进制星类是否包括与不同超新星形成途径相关的不同亚群.
- 为了确定这些潜在的子群体之间的可观察到的差异.
主要方法:
- 在Be/X射线双星中分析中子星的特征旋转周期,轨道周期和轨道偏心.
- 这些参数的统计比较以确定不同的分组.
主要成果:
- 一大类中子星宿主X射线脉冲星 (Be/X射线二进制星) 被发现由两个不同的子群组成.
- 这些子群体在它们的特征旋转周期,轨道周期和轨道异常度上有所不同.
- 电子捕获超新星最好与表现出短旋转周期,短轨道周期和低离心率的系统相关.
结论:
- 在Be/X射线双星中观察到的子群可能与两个不同的超新星形成通道相对应.
- 电子捕获超新星可能会产生具有特定特性 (较短周期,较低离心率) 的中子星.
- 旋转周期分布对数的明显分割是意想不到的,需要进一步的理论解释.
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