一颗热白矮星的合并残留物,通过对碳的紫外线检测而揭示出来
Snehalata Sahu1, Antoine Bédard1, Boris T Gänsicke1
1Department of Physics, University of Warwick, Coventry, UK.
概括
天文学家在白矮星中检测到低水平的碳,揭示它是恒星合并残留物. 这一发现凸显了紫外线光谱对于发现这些物体的重要性.
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 白矮人的研究 白矮人的研究
背景情况:
- 超大质量白矮星具有高碳丰度以前使用光学光谱学识别.
- 这些物体被认为起源于恒星的合并,并与热核超新星有关.
- 光学方法只能检测到最富含碳的白矮星,可能缺少其他合并残留物.
研究的目的:
- 用紫外线光谱学研究富含的超大质量白矮星WD 0525+526的大气组成.
- 根据其大气特性,确定WD 0525+526是否是恒星合并残余.
- 探索外结构在白矮星大气组成中的作用.
主要方法:
- 使用哈勃太空望远镜进行远紫外光谱学.
- 在WD 0525+526.6中对大气碳丰度的分析.
- 白矮星外结构和进化的建模.
主要成果:
- 在WD 0525+526中检测到大气中的碳含量明显低于之前观察到的白矮星 (log(C/H) = -4.62).
- 气和气外的质量远低于单一恒星进化的预期,支持一个合并起源.
- 推断出一个独特的包裹结构,在半对流区上有一层薄的层.
结论:
- WD 0525+526被确定为恒星合并残余,与以前已知的富含碳的白矮星不同.
- 紫外线光谱对于检测较少碳丰富的聚合残留物至关重要.
- 这项研究强调了被忽视的外结构在理解白矮星演变中的重要性.
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