The evolution of mass loaded supernova remnants - I. Constant and Mach Number dependent mass injection rates

The evolution of mass loaded supernova remnants - I. Constant and Mach Number dependent mass injection rates
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质量加载超新星遗迹的演化 - I. 恒定和马赫数相关的质量注入速率

DOI:
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发表时间:
2002
期刊:
影响因子:
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通讯作者:
T. Hartquist
T. Hartquist
中科院分区:
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文献类型:
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作者:
J. Dyson;S. J. Arthur;T. Hartquist

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我们描述了球对称超新星残骸的演化,其中质量的增加发生在嵌入的云中。我们推导了遗迹演化的简单近似,可用于研究超新星引起的现象,如星系超风的产生。
We describe the evolution of spherically symmetric supernova remnants in which mass addition takes place from embedded clouds. We derive simple approximations to the remnant evolution which can be used for investigating the generation of supernova induced phenomena such as galactic superwinds.