靠近的黑洞双星V404 Cygni的快速光学变化的重复模式
Mariko Kimura1, Keisuke Isogai1, Taichi Kato1
1Department of Astronomy, Graduate School of Science, Kyoto University, Oiwakecho, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan.
Nature
|January 8, 2016
概括
在像V404天这样的黑洞系统中, 这挑战了以前关于积累盘不稳定的理论.
科学领域:
- 天体物理学
- 黑洞研究
- 收缩磁盘动力学
背景情况:
- 黑洞的积累机制仍然不太清楚.
- 收缩盘被认为是X射线变异的原因,特别是在埃丁顿极限附近.
- 之前的观测将大振幅振荡与高质量增量率联系起来.
研究的目的:
- 调查黑洞系统中大振幅光学振荡的原因.
- 确定诱导内部磁盘不稳定的关键参数.
- 重新评估质量增加率与其他因素的作用.
主要方法:
- 对V404 Cygni进行了广泛的多色光学光度数据分析.
- 观察到的振荡与质量增加率和轨道周期的比较.
- 对二进制系统中的积累盘行为进行理论建模.
主要成果:
- 在100秒到2.5小时的时间范围内观察到大幅度的光学振荡.
- 这些波动发生的质量增加率明显低于此前的假设.
- 长的轨道周期被确定为这些振荡的关键条件.
结论:
- 质量积累率不是内盘不稳定的唯一关键参数.
- 长的轨道周期,导致外盘的表面密度较低,至关重要.
- 在长期系统中,持续积累的缺乏,而不是速度本身,很可能是驱动这些振荡的原因.
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