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Observational constraints on the progenitor of core-collapse supernovae

Date Issued
2016
Author(s)
DOI
Abstract
It is well-known that some massive stars evolve to an end state which results in the collapse of the stellar core, as the hydrostatic pressure can no longer support gravity, leading to powerful explosions called supernovae (SNe). Even with over 6000 known SNe, we have only direct information about the progenitor star for a handful of explosions. Here, I summarise the observational constraints of the massive progenitor stars of several core-collapse supernovae.
Coverage
XXIX General Assembly
Series
Volume
vol. 11, A29B (Astronomy in Focus)
Start page
209
Uri
Url
Issn Identifier
1743-9213
Ads BibCode
2016IAUFM..29B.209E
Rights
open.access
File(s)
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2016IAUFM_29B_209E.pdf

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Format

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