Wind driven mass transfer in interacting binary systems
Wind driven mass transfer in interacting binary systems
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DOI：
10.1093/mnras/253.1.9
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发表时间：
1991-11
影响因子：
4.8
通讯作者：
C. Tout;D. Hall
中科院分区：
文献类型：
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作者：
C. Tout;D. Hall
密近双星系统中的恒星可能会经历两种质量变化：1）恒星之间的质量转移，以及2）系统的质量完全损失。前一个过程发生在一颗恒星充满它的洛希瓣时，而后者可能是以恒星风的形式出现。当这两者同时存在时，观测估计表明质量传递速率和质量损失速率是相同的数量级。对于这种相似性的一个简单的解释可以找到，如果质量损失，由恒星风，从罗氏填充星星是背后的驱动机制质量转移
Stars in close binary systems can suffer two kinds of mass change : 1) mass transfer between the stars, and 2) mass loss completely from the system. The former process occurs when one the stars fills its Roche lobe while the latter may be in the form of a stellar wind. When both of these exist together, observational estimates indicate that the mass-transfer rate and the mass-loss rate are of the same order. A simple explanation for this similarity can be found if the mass loss, by stellar wind, from the Roche filling star is the driving mechanism behind mass transfer