在A型恒星和白矮星中发现磁场的化石起源
Jonathan Braithwaite1, Hendrik C Spruit
1Max-Planck-Institute for Astrophysics, Postfach 1317, 85741 Garching, Germany.
Nature
|October 16, 2004
概括
在Ap星,磁性白矮星和磁星中强大的恒星磁场可能是化石场. 数字模拟表明这些稳定的场可以从不稳定的初始状态演变,统一它们的解释.
科学领域:
- 天文学和天体物理学
- 恒星磁力 恒星磁力是什么
- 计算物理 计算物理
背景情况:
- 一些主要序列恒星 (Ap恒星) 呈现强烈的,静态的,大规模的双极磁场.
- 存在两种假设:化石场 (形成的残留物) 或动力发电机过程.
- 动力发电机假设努力解释场强度和旋转相关性缺乏.
研究的目的:
- 研究恒星磁场的稳定性和演变.
- 为了确定化石场是否可以解释恒星中观察到的磁场特性.
- 为不同类型的恒星提供一个统一的恒星磁性的解释.
主要方法:
- 磁场演变的数值模拟.
- 模拟从任意的初始场发展稳定的磁性配置.
- 将模拟结果与Ap星,磁性白矮星和磁星的观测数据进行比较.
主要成果:
- 模拟表明,稳定的磁场配置可以从不稳定的初始磁场中发展.
- 模拟的稳定场与观察到的恒星磁场的属性相匹配.
- 这些发现支持化石场理论对这些恒星的动力发电机产生.
结论:
- 化石场是Ap星,磁性白矮星和磁星中观察到的强磁场的可行和统一的解释.
- 稳定的磁性配置可以自然地从进化过程中产生的.
- 这项研究解决了关于恒星磁性的起源的长期问题.
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