相关实验视频
Updated: Jun 23, 2026

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Hyperpolarized Xenon for NMR and MRI Applications
Published on: September 6, 2012
一个无线电脉冲星/X射线二元链接
Anne M Archibald1, Ingrid H Stairs, Scott M Ransom
1Department of Physics, McGill University, 3600 Rue University, Montréal, Quebec, H3A 2T8, Canada. aarchiba@physics.mcgill.ca
概括
研究人员在一个二进制星系中检测到附近的无线电毫秒脉冲星 (MSP). 这一发现表明脉冲星最近从低质量X射线二进制 (LMXB) 阶段过渡,这是目前没有增积盘的迹象.
科学领域:
- 天文学和天体物理学
- 紧的对象 紧的对象
- 二进制系统二进制系统
背景情况:
- 毫秒脉冲星 (MSP) 是快速旋转的中子星,据信是由伴星的质量转移旋转而形成的.
- 低质量X射线二进制 (LMXB) 系统是MSP的理论祖先,但直接的观测联系仍然难以捉摸.
- 之前在LMXB中寻找无线电脉冲的搜索没有产生明确的检测结果.
研究的目的:
- 报告发现了一个新的无线电毫秒脉冲星 (MSP).
- 为了调查附近的MSP系统与光学识别的伴侣的进化状态.
- 探索从低质量X射线双星 (LMXB) 阶段到活跃射电脉冲星阶段的过渡.
主要方法:
- 来自毫秒脉冲星的无线电脉冲的检测.
- 后续观察包括光学光度测量和光谱学.
- 分析光学数据以确定增积盘的存在或不存在.
主要成果:
- 一个附近的无线电毫秒脉冲星 (MSP) 被成功检测和观察.
- 该系统表现出一个圆形的二进制轨道与一个光学识别的伴星.
- 光学观测表明,最近一个积累盘消失了,这表明质量转移已经停止.
结论:
- 检测到的无线电MSP可能从低质量X射线二进制 (LMXB) 阶段过渡.
- 没有当前的积累盘表明最近的LMXB阶段.
- 这一发现为毫秒脉冲星形成的旋转模型提供了观察证据.
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