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Progenitors of Core-Collapse Supernovae

Published online by Cambridge University Press:  17 October 2017

R. Hirschi ,
D. Arnett ,
A. Cristini Open the ORCID record for A. Cristini [Opens in a new window] ,
C. Georgy Open the ORCID record for C. Georgy [Opens in a new window] ,
C. Meakin  and
I. Walkington
R. Hirschi
Affiliation:
Astrophysics Group, Keele University, Lennard-Jones Laboratories, Keele, ST5 5BG, UK email: [email protected] Kavli IPMU (WPI), The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
D. Arnett
Affiliation:
Department of Astronomy, University of Arizona, Tucson, AZ 85721, USA
A. Cristini
Affiliation:
Astrophysics Group, Keele University, Lennard-Jones Laboratories, Keele, ST5 5BG, UK email: [email protected]
C. Georgy
Affiliation:
Geneva Observatory, University of Geneva, Ch. Maillettes 51, 1290 Versoix, Switzerland
C. Meakin
Affiliation:
Department of Astronomy, University of Arizona, Tucson, AZ 85721, USA Karagozian & Case, Inc., 700 N. Brand Blvd. Suite 700, Glendale, CA, 91203, USA
I. Walkington
Affiliation:
Astrophysics Group, Keele University, Lennard-Jones Laboratories, Keele, ST5 5BG, UK email: [email protected]
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Abstract

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Massive stars have a strong impact on their surroundings, in particular when they produce a core-collapse supernova at the end of their evolution. In these proceedings, we review the general evolution of massive stars and their properties at collapse as well as the transition between massive and intermediate-mass stars. We also summarise the effects of metallicity and rotation. We then discuss some of the major uncertainties in the modelling of massive stars, with a particular emphasis on the treatment of convection in 1D stellar evolution codes. Finally, we present new 3D hydrodynamic simulations of convection in carbon burning and list key points to take from 3D hydrodynamic studies for the development of new prescriptions for convective boundary mixing in 1D stellar evolution codes.

Keywords

convectionstars: evolutioninteriorsrotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S331: Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their aftermaths , February 2017 , pp. 1 - 10
Copyright
Copyright © International Astronomical Union 2017 

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