由费米LAT揭示的超新星残骸W44外的马射线辐射
A A Abdo1, M Ackermann, M Ajello
1Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA.
概括
像W44这样的超新星残留物加速宇宙射线,产生马射线辐射. 观测证实了质子和原子核是源头,为宇宙中的粒子加速提供了洞察力.
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
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 超新星残留物 (SNRs) 被假设加速宇宙射线到极高的能量.
- 负责从SNR观察到的辐射的特定颗粒仍然未被确定.
研究的目的:
- 调查SNR W44.4.高能排放的来源.
- 在SNR中识别负责马射线生成的粒子.
- 探测粒子加速机制及其环境依赖性.
主要方法:
- 使用费米大面积望远镜观测SNR W44.
- 分析2 x 10^8到3 x 10^11电子伏特的能量范围内的马射线光谱.
- 玛射线源和SNR外之间的形态比较.
主要成果:
- 探测到一个与SNR W44外空间一致的马射线源.
- 马射线光谱是通过质子和原子核的辐射很好地建模出来的.
- 在大约10^9电子伏特以上观察到光谱度.
结论:
- 来自SNR W44的马射线辐射是由残留物中加速的粒子产生的.
- 质子和原子核是这种辐射的可能来源.
- 光谱特征提供了关于粒子在密集环境中的加速及其释放到星际空间的见解.
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