吉明加的尾巴:一个脉冲星的弓冲击探测星际介质
P A Caraveo1, G F Bignami, A DeLuca
1Istituto di Astrofisica Spaziale e Fisica Cosmica-Consiglio Nazionale della Richerche, Via Bassini, 15-20133 Milano, Italy. pat@mi.iasf.cnr.it
概括
X射线观测揭示了两个平行尾巴跟着脉冲星Geminga,由其超音速运动引起. 这种脉冲星弓冲击探测提供了对电子能量和磁场的洞察.
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
- 血物理学的等离子体物理学
背景情况:
- 脉冲星是快速旋转的中子星,它们会发出辐射束.
- 脉冲风星云是由脉冲风与星际介质的相互作用形成的.
- 杰明加是一个靠近的,孤立的中子星.
研究的目的:
- 为了研究与脉冲星Geminga相关的观察到的X射线尾巴的性质.
- 分析X射线尾的发射机制和物理特性.
- 使用脉冲星弓冲击的X射线检测来限制天体物理参数.
主要方法:
- 使用了来自X射线多反射镜任务-牛顿欧洲光子成像摄像机 (EPIC) 的数据.
- 分析了长长的X射线尾巴的形态和光谱特性.
- 在弓形冲击结构中模拟了电子同步子发射.
主要成果:
- 观察到两个平行X射线尾巴跟着金刚,与其超音速运动保持一致.
- 尾部呈现出非热频谱,表明电子同步子发射.
- 电子冷却时间与通过观察到的X射线特征的传输时间相匹配.
结论:
- X射线尾巴代表了一个脉冲星弓冲击,由Geminga的风与星际介质相互作用而形成.
- 这种检测允许估计脉冲星的电子注入能量和冲击的磁场.
- 限制了Geminga的运动角度和周围局部物质的密度.
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