Interaction of Supernovae with Circumstellar Matter
Interaction of Supernovae with Circumstellar Matter
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DOI：
10.1007/978-1-4612-3286-5_5
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发表时间：
1990
期刊：
影响因子：
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通讯作者：
R. Chevalier
中科院分区：
文献类型：
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作者：
R. Chevalier
众所周知，基本上所有质量的恒星在演化过程中都会失去质量。恒星在任何时刻的质量损失特性是由恒星的演化状态决定的。被这些过程改变的恒星周围的区域被称为星周介质。除了单星的质量损失外，双星系统中的质量传递和质量损失也可能在决定恒星周围环境方面发挥作用。
Stars of essentially all masses are known to lose mass during their evolution. The mass loss characteristics at any time are determined by the evolutionary status of the star. The region around a star that is modified by these processes is referred to as the circumstellar medium. In addition to mass loss from a single star, mass transfer and mass loss in a binary system may play a role in determining the circumstellar environment.