两个白矮星具有富含氧气的大气层
B T Gänsicke1, D Koester, J Girven
1Department of Physics, University of Warwick, Coventry CV4 7AL, UK. Boris.Gaensicke@warwick.ac.uk
概括
巨大的恒星 (7-10太阳质量) 可以形成氧气白矮星. 这些发现为恒星进化路径提供了观测证据,避免了核心崩的超新星.
科学领域:
- 天文学和天体物理学.
- 恒星进化中的恒星演变
- 白矮星是一颗白矮星.
背景情况:
- 恒星的质量在7-10太阳质量之间,其进化终点不确定.
- 这些终点是巨大的白矮星或弱型II超新星.
- 这些路径的观测约束是有限的.
研究的目的:
- 为了研究大质量恒星的进化路径.
- 为了确定避免核心崩的恒星的观测特征.
- 为了限制大质量白矮星的形成.
主要方法:
- 检测具有特定光球丰度的白矮星.
- 分析恒星大气中的氧气丰度.
- 在恒星进化模型中解释发现.
主要成果:
- 发现了两颗具有高光圈氧气丰度的白矮星.
- 这些白矮星被确定为裸体的氧气虹核.
- 这表明它们起源于大规模的祖先,这些祖先避免了核心崩.
结论:
- 巨大的恒星可以演变为氧气虹白矮星.
- 这为特定的恒星死亡途径提供了观测证据.
- 这些发现有助于限制中等质量恒星的恒星演变模型.
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