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一颗旋转的白矮星在对面呈现不同的组成
Ilaria Caiazzo1, Kevin B Burdge2,3, Pier-Emmanuel Tremblay4
1Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA. ilariac@caltech.edu.
Nature
|July 19, 2023
概括
天文学家发现了一个独特的白矮星,ZTF J203349.8+322901.1,它的大气层一侧由,另一侧由组成. 这颗"双面"的恒星提供了关于恒星进化和磁场对白矮星的影响的新见解.
科学领域:
- 恒星天体物理学
- 白矮人的进化
- 星球科学
背景情况:
- 白矮星是密集的恒星残骸,质量与太阳相似,大小与地球相似.
- 引力沉积导致重元素沉下,在大气中留下轻元素如或.
- 白矮星大气层从气转变为气,因为它们的温度低于3万克尔文.
研究的目的:
- 报告发现和观察一个独特的白矮星, ZTF J203349.8+322901.
- 调查其独特的双面大气组成 (和) 的原因.
- 探索磁场在白矮星光谱演变中的作用.
主要方法:
- 使用先进望远镜捕获光谱数据的观测天文学.
- 对大气组成和白矮星表面温度变化的分析.
- 与现有的白矮星冷却和磁场效应模型进行比较.
主要成果:
- 发现ZTF J203349.8+322901.1,一个具有明显和主导的大气区域的白矮星.
- 观察到的不均性可能是由弱磁场影响表面条件造成的.
- 这一发现表明ZTF J203349.8+322901.1是磁性转变白矮星的一个极端例子.
结论:
- ZTF J203349.8+322901.1的存在为磁场影响白矮星大气组成提供了强有力的证据.
- 这一发现有助于理解白矮星的光谱演变.
- 进一步研究这一类磁性白矮星可以揭示基本的恒星过程.
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