检测柔软的X射线和敏感的寻找珍贵气体的彗星海尔-波普彗星
V A Krasnopolsky1, M J Mumma, M Abbott
1Catholic University of America, Washington, DC 20064, USA. ys2VK@lepvax.gsfc.nasa.gov 20771, USA.
概括
哈雷-波普彗星的彗星
科学领域:
- 彗星科学是一门彗星科学.
- X射线天文学X射线天文学
- 天体化学是天体化学.
背景情况:
- 海尔-波普彗星 (C/1995 O1) 是一种在软X射线中观察到的突出的彗星.
- 之前的观测缺乏对其X射线辐射和元素组成的详细分析.
研究的目的:
- 为了分析黑尔-波普彗星的软X射线辐射.
- 为了确定彗星冰的元素组成.
- 为了研究彗星冰的形成条件.
主要方法:
- 黑尔波普彗星的软X射线成像.
- 对X射线辐射的光谱分析.
- 与太阳能丰度和理论模型进行比较.
主要成果:
- 检测到X射线辐射,其中一个中心特征与核相抵消,一个扩展的特征与尘埃喷射无关.
- 与太阳丰富相比,虹灯的耗尽超过25倍.
- 检测了584安格斯特罗姆的线辐射,可能来自太阳风的电荷转移.
- 在538安格斯特罗姆的辐射的观测归因于电离氧和.
结论:
- 黑尔-波普彗星中的彗星冰可能是在高于25克尔文的温度下形成的.
- 太阳风的相互作用在彗星的X射线辐射中起作用.
- X射线观测为彗星的组成和过程提供了独特的见解.
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