准确的几何距离到紧的双星SS Cygni证明了增积盘理论的正确性
J C A Miller-Jones1, G R Sivakoff, C Knigge
1International Centre for Radio Astronomy Research, Curtin University, Perth, WA 6845, Australia. james.miller-jones@curtin.edu.au
概括
精确的距离测量显示,SS Cygni比以前认为的更近. 这一发现解决了对矮星新星的积累盘理论的一个重大挑战.
科学领域:
- * 天体物理学 * 天体物理学
- * 恒星演变的过程
- * 积累物理学的积累物理
背景情况:
- *矮星新星是带有白矮星从红矮星中增加物质的双星系统.
- * 它们的爆发是由磁盘不稳定模型解释的.
- * 矮星新星SS Cygni由于其先前估计的亮度挑战了这个模型.
研究的目的:
- *为了准确地确定距离SS Cygni的距离.
- *为了使SS Cygni的观察行为与增积盘理论相协调.
- * 解决了解紧物体中的积累的差异.
主要方法:
- *采用了非常长的基线干扰计 (VLBI) 无线电观测.
- * 用一种独立于模型的方法来确定距离.
- * 集成精确的抛物线测量.
主要成果:
- * 确定了一个新的,准确的距离SS Cygni的114±2帕塞克.
- *这个修订后的距离比之前的哈勃太空望远镜估计的159 ± 12帕塞克要近得多.
- *新的距离解决了SS Cygni爆发的亮度悖论.
结论:
- *对SS Cygni的修订距离使其行为与磁盘不稳定性模型保持一致.
- * 这项研究加强了对紧物体的积累盘理论的有效性.
- *精确的距离测量对于理解天体物理现象至关重要.
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