用费米大面积望远镜观测到的一群马射线毫秒脉冲星
A A Abdo1, M Ackermann, M Ajello
1Space Science Division, Naval Research Laboratory,Washington, DC 20375, USA.
概括
双星系统中的毫秒脉冲星 (MSP) 可以重新获得"第二次生命",旋转以发射可检测的马射线脉冲. 这些发现表明MSP和年轻脉冲星之间存在共同的发射机制.
科学领域:
- * 天文学和天体物理学
- * 高能天体物理学
- * 中子星物理学
背景情况:
- *脉冲星是快速旋转的中子星,它们发出电磁辐射束.
- *最初,脉冲星由于数百万年的电磁制动而旋转下降.
- * 双星系统中的中子星可以积聚物质,从而以毫秒脉冲星 (MSP) 的形式产生"第二次生命".
研究的目的:
- * 为了寻找已知的毫秒脉冲星 (MSPs) 在球状星团之外的马射线脉冲.
- * 为了研究回收脉冲星的排放特性.
- * 将MSP的特征与年轻,充满活力的脉冲星的特征进行比较.
主要方法:
- *使用了费米大面积望远镜 (LAT) 的数据.
- *使用了从射电望远镜观测中获得的旋转参数.
- *分析了马射线数据,以检测MSP样本中的脉冲.
主要成果:
- * 检测到八个先前已知的MSP的显著马射线脉冲.
- * 观察到这些MSP的马射线脉冲形状和光谱特性与年轻的马射线脉冲星相似.
- *确定了MSP和年轻脉冲星之间的排放机制的相似之处.
结论:
- *毫秒脉冲星表现出与年轻脉冲星共享的共同发射机制相一致的特性.
- *MSP和年轻脉冲星中的辐射似乎来自远离中子星表面的区域.
- *这项研究强调了二进制相互作用在中子星的进化和可观测性质中的重要性.
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