期刊
ROYAL SOCIETY OPEN SCIENCE
卷 7, 期 7, 页码 -出版社
ROYAL SOC
DOI: 10.1098/rsos.200467
关键词
supernovae; massive stars; mass loss
资金
- Royal Society - Science Foundation Ireland University Research Fellowship
It is 30 years since the characteristic signatures of interaction with circumstellar material (CSM) were first observed in a core-collapse supernova. Since then, CSM interaction has been observed and inferred across a range of transients, from the low-energy explosions of low-mass stars as likely electron-capture supernovae, through to the brightest superluminous supernovae. In this review, I present a brief overview of some of the interacting supernovae and transients that have been observed to date, and attempt to classify and group them together in a phenomenological framework.
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