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Core-Collape Supernova Progenitors: Light-Curve and Stellar-Evolution Models

Published online by Cambridge University Press:  28 July 2017

Melina C. Bersten
Melina C. Bersten*
Affiliation:
Instituto de Astrofísica de La Plata (IALP), CCT-CONICET-UNLP. Paseo del Bosque S/N (B1900FWA), La Plata, and Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Argentina, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan email: mbersten@fcaglp.unlp.edu.ar
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Abstract

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A very active area of research in the field of core-collapse supernovae (SNe) is the study of their progenitors and the links with different subtypes. Direct identification using pre- and post-SN images is a powerful method but it can only be applied to the most nearby events. An alternative method is the hydrodynamical modeling of SN light curves and expansion velocities, which can serve to characterize the progenitor (e.g. mass and radius) and the explosion itself (e.g. explosion energy and radioactive yields). This latter methodology is particularly powerful when combined with stellar evolution calculations. We review our current understanding of the properties of normal core-collapse SNe based chiefly on these two methods.

Keywords

binaries: generalsupernovae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 25 - 31
Copyright
Copyright © International Astronomical Union 2017 

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