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在白矮星中,强磁场抑制了冷却
G Valyavin1, D Shulyak2, G A Wade3
1Special Astrophysical Observatory of Russian Academy of Science, Nizhnij Arkhyz, Zelenchukskiy region, Karachai-Cherkessian Republic 369167, Russia.
Nature
|October 21, 2014
概括
由于抑制了冷却,具有强磁场的冷白矮星看起来更年轻. 这种磁场效应解释了为什么较老,较冷的白矮星通常表现出强烈的磁场,从而解决了长期存在的天文学难题.
科学领域:
- 天文学 天文学
- 恒星天体物理学 恒星天体物理学
- 磁动力学是一种磁动力学.
背景情况:
- 凉爽的白矮星往往具有强大的磁场,与随着时间的推移场衰减的预期相反.
- 磁性白矮星的亮度变化归因于表面不均性和磁光学效应.
研究的目的:
- 为了研究冷白矮星中磁场和大气特性之间的关系.
- 为了解释较冷的白矮星中强磁场的普遍存在.
主要方法:
- 对白矮星WD的亮度和磁场的长期光学观测 1953-011.11.
- 对表面温度和磁场分布的分析.
主要成果:
- 强大的磁场抑制了白矮星中的大气对流.
- 抑制的对流会导致高度磁化区域的暗点.
- 磁场抑制了冷白矮星的冷却演变.
结论:
- 磁场抑制对流解释了冷白矮星中强磁场的普遍存在.
- 这种机制使强磁性的白矮星看起来比其实际年龄更年轻.
- 目前对强磁白矮星的年龄估计可能被系统地低估.
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