马射线发射与共生双星V407天星中的新星并发
1, A A Abdo, M Ackermann
1Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA.
概括
天文学家检测到来自新星V407 Cygni的意想不到的马射线辐射,挑战了以前的模型. 这个新星是新星.
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
- 恒星进化中的恒星演变
背景情况:
- 新星是由于白矮星的积累而产生的恒星爆炸.
- 预计新星会发射X射线,但更高能量的辐射不会.
- V407天是一个共生恒星系统,最近出现了一颗光学新星.
研究的目的:
- 报告从新星V407 Cygni. 探测到的马射线辐射.
- 为了调查这种意想不到的高能排放的起源.
主要方法:
- 费米大面积望远镜的观测结果.
- 分析可变的马射线发射 (0.1到10 GeV).
主要成果:
- 从V407 Cygni.检测到可变的马射线辐射.
- 排放的能量范围从0.1到10GeV.
结论:
- 拟议的机制:新星外与红巨人的密集介质的相互作用加速粒子.
- 质子-质子相互作用可能产生pi(0) 衰变的马射线.
- 红巨星辐射的反复康普顿散射是一种可能的,虽然未被证实的发射源.
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