期刊
ASTRONOMY & ASTROPHYSICS
卷 390, 期 3, 页码 1063-1074出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20020731
关键词
ISM : kinematics and dynamics; ISM : supernova remnants; galaxies : ISM
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.
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