来自超新星1987A残余中的紧物体的电离辐射排放线
C Fransson1, M J Barlow2, P J Kavanagh3,4
1Department of Astronomy, Stockholm University, The Oskar Klein Centre, AlbaNova, SE-106 91 Stockholm, Sweden.
概括
天文学家使用JWST光谱观测超新星1987A,检测出辐射线表明像中子星这样的紧物体. 这一发现可能为中子星的出生提供了证据.
科学领域:
- 天体物理学
- 观测天文学
背景情况:
- 超新星1987A产生了中微子,表明形成了一个紧的物体 (中子星或黑洞).
- 自超新星事件发生以来, 这颗紧的天体还没有被直接观测到.
研究的目的:
- 在超新星1987A中形成的紧物体直接观察.
- 调查紧物体的性质及其对超新星残留物的潜在影响.
主要方法:
- 利用詹姆斯·韦伯太空望远镜 (JWST) 的光谱观测超新星1987A的残余物.
- 在残留物中分析了和硫的狭窄红外辐射线.
主要成果:
- 检测到空间未解决,蓝移红外辐射线的和硫.
- 这些线条源于中央气体的电离.
- 线比与冷却中的中子星或脉冲风星云的电离相一致.
结论:
- 观察到的辐射线表明在超新星残余的中心存在一个紧的物体.
- 辐射线的速度转移可能表明中子星在形成过程中被赋予了出生.
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