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Observational constraints on the progenitor of core-collapse supernovae

Published online by Cambridge University Press:  27 October 2016

Nancy Elias-Rosa
Nancy Elias-Rosa*
Affiliation:
INAF - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova I-35122, Italy email: [email protected]
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Abstract

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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.

Keywords

(stars:) supernovae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 209 - 210
Copyright
Copyright © International Astronomical Union 2016 

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