DYNAMICAL EVOLUTION OF SUPERNOVA REMNANTS BREAKING THROUGH MOLECULAR CLOUDS
We carry out three-dimensional hydrodynamic simulations of the supernova remnants (SNRs) produced inside molecular clouds (MCs) near their surface using the HLL code \citep{har83}. We explore the dynamical evolution and the X-ray morphology of SNRs after breaking through the MC surface for ranges of...
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| Published in | Journal of The Korean Astronomical Society Vol. 48; no. 2; pp. 139 - 154 |
|---|---|
| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
한국천문학회
30.04.2015
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| Subjects | |
| Online Access | Get full text |
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