一颗有氧气层的白矮星
S O Kepler1, Detlev Koester2, Gustavo Ourique3
1Instituto de Física, Universidade Federal do Rio Grande do Sul, 91501-900 Porto Alegre, RS, Brazil. kepler@if.ufrgs.br.
概括
天文学家发现了一颗独特的白矮星, 这一发现挑战了典型的白矮星大气模型,
科学领域:
- 天文学与天体物理学
- 恒星进化
- 白矮星
背景情况:
- 由于引力扩散,白矮星通常具有由和等轻元素主导的大气层.
- 预计初始质量低于大约10个太阳质量的恒星将演变成白矮星.
研究的目的:
- 报道发现一个不寻常的白矮星, SDSS J124043.01+671034.68.
- 描述这颗独特的白矮星的大气组成, 并研究它对恒星进化的影响.
主要方法:
- 白矮星SDSS J124043.01+671034.68的光谱分析
- 对恒星大气的组成分析以确定元素的丰度.
主要成果:
- 白矮星SDSS J124043.01+671034.68的大气几乎完全由氧气组成.
- 尼和的含量至少低于氧气的25倍.
- 在恒星大气层中没有发现或.
结论:
- 观测到的大气组成表明这颗白矮星可能是氧气类型.
- 这一发现为恒星演变模型提供了一个罕见的观测测试,特别是对于白矮星形成前更大质量的恒星.
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