Modeling the signatures of interaction in Type II supernovae: UV emission, high-velocity features, broad-boxy profiles
Because mass loss is a fundamental phenomenon in massive stars, an interaction with circumstellar material (CSM) should be universal in core-collapse supernovae (SNe). Leaving aside the extreme CSM density, extent, or mass typically encountered in Type IIn SNe, we investigate the diverse long-term r...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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EDP Sciences
2022
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| Online Access: | View Fulltext in Publisher |