一颗燃烧的白矮星作为超软X射线源
J Greiner1, C Maitra2, F Haberl2
1Max-Planck-Institut für extraterrestrische Physik, Garching, Germany. jcg@mpe.mpg.de.
Nature
|March 23, 2023
概括
研究人员发现了一种新的超软X射线源, 这种积的白矮星系统为恒星爆炸和铁等元素的起源提供了新的见解.
科学领域:
- * 天体物理学
- * 恒星进化
- * 超新星
背景情况:
- 一类超新星是重要的宇宙距离标记和主要的铁源.
- 目前的Ia型超新星原始模型难以解释观测数据.
- * 存在积白矮星作为祖先已经被理论化,但没有观察到.
研究的目的:
- 报告发现了一种新型的超软X射线源.
- 为了研究它作为Ia型超新星的祖先的潜力.
- 探索恒星爆炸和元素合成的新途径.
主要方法:
- * 一个超软的X射线源的观察.
- * 它的积累盘的光谱分析.
- * 对X射线和光学辐射的解释
主要成果:
- * 检测出一种超软的X射线源,其中占主导地位.
- 在白矮星表面有稳定的燃烧的证据.
- * 该系统的属性与积白矮星祖先的预测一致.
结论:
- * 观察到的系统提供了积白矮星作为Ia型超新星的第一个直接证据.
- 这一发现支持了Chandrasekhar质量爆炸的延伸路径.
- 这可能解释了亚能量型Iax超新星的起源.
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