一个"非磁性"白矮星的磁门积累
S Scaringi1, T J Maccarone2, C D'Angelo3
1School of Physical and Chemical Sciences, University of Canterbury, Christchurch 8041, New Zealand.
Nature
|December 15, 2017
概括
研究人员在一个"非磁性"白矮星双星系统MV Lyrae中发现了磁门积累. 这一发现揭示了研究白矮星磁场及其积聚过程的新方法.
科学领域:
- 天体物理学
- 恒星进化
- 二进制系统
背景情况:
- 双星系统中的白矮星从伴星中积聚气体,大约有15%的情况是强磁场引导物质.
- 缺乏强磁场影响积累的系统被称为"非磁性".
- 白矮星的积聚过程对于理解恒星进化和Ia型超新星等现象至关重要.
研究的目的:
- 为了研究"非磁性"白矮星双星系统MV Lyrae的积累动态.
- 确定磁场是否在以前被认为非磁性的系统中起作用.
- 建立一种新的方法来推断白矮星的磁场强度.
主要方法:
- 对MV Lyrae二进制星系的存档光学观测进行分析.
- 检查光线曲线的特征爆发模式.
- 基于观察到的爆发时间和振幅的积累模式的建模.
主要成果:
- MV Lyrae表现出半周期性爆发 (30分钟持续,每2小时),表明不稳定的,磁调节的积累模式.
- 磁门积累的证据,磁盘材料在积累之前在协同旋转半径上积累.
- 推断白矮星表面磁场强度为2x10^4到1x10^5高斯,低于当前的直接检测极限.
结论:
- 这项研究证明了"非磁性"白矮星的磁性积,挑战了以前的分类.
- 这一发现为测量白矮星中的磁场提供了一种新的方法.
- 它加强了白矮星,年轻恒星物体和中子星的积聚现象之间的联系.
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