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Early Emission of Core-Collapse Supernovae

Published online by Cambridge University Press:  29 January 2014

Melina C. Bersten ,
Omar Benvenuto  and
Ken'ichi Nomoto
Melina C. Bersten
Affiliation:
Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan email: melina.bersten@ipmu.jp
Omar Benvenuto
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, B1900FWA La Plata, Argentina email: obenvenu@fcaglp.unlp.edu.ar
Ken'ichi Nomoto
Affiliation:
Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan email: melina.bersten@ipmu.jp
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Abstract

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We present a study of the early UV/Optical emission of the stripped-envelope supernovae based on a one-dimensional, Lagrangian model that solves the hydrodynamics and radiation transport in an expanding ejecta. The models are compared with observations to constrain the physical properties of the progenitor star, such as radius and mixing of radioactive nickel synthesized during the explosion. In particular, we present models for the early emission of the type IIb SN 2011dh and the Type Ib SN 2008D.

Keywords

supernovae: generalsupernovae: individual (SN 2008D)supernovae: individual (SN 2011dh)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 58 - 62
Copyright
Copyright © International Astronomical Union 2014 

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