Radiation-Driven Stellar Eruptions
Very massive stars occasionally expel material in colossal eruptions, driven by continuum radiation pressure rather than blast waves. Some of them rival supernovae in total radiative output, and the mass loss is crucial for subsequent evolution. Some are supernova impostors, including SN precursor o...
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| Format: | Article |
| Language: | English |
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MDPI AG
2020-02-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/8/1/10 |