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Supernova Yields for Chemical Evolution Modeling

Published online by Cambridge University Press:  06 January 2014

Ken'ichi Nomoto  and
Tomoharu Suzuki
Ken'ichi Nomoto
Affiliation:
Kavli Institute for the Physics and Mathematics of the Universe (WPI) The University of Tokyo, Kashiwa, Chiba 277-8583, Japan email: nomoto@astron.s.u-tokyo.ac.jp
Tomoharu Suzuki
Affiliation:
College of Engineering, Chubu University, Kasugai, Aichi 487-8501, Japan email: tsuzuki@isc.chubu.ac.jp
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Abstract

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We review the recent results of the nucleosynthesis yields of massive stars. We examine how those yields are affected by some hydrodynamical effects during the supernova explosions, namely, explosion energies from those of hypernovae to faint supernovae, mixing and fallback of processed materials, asphericity, etc. Those parameters in the supernova nucleosynthesis models are constrained from observational data of supernovae and metal-poor stars. The elemental abundance patterns observed in extremely metal-poor stars show some peculiarities relative to the solar abundance pattern, which suggests the important contributions of hypernovae and faint supernovae in the early chemical enrichment of galaxies. These constraints on supernova nucleosynthesis are taken into account in the latest yield table for chemical evolution modeling.

Keywords

stars: abundancesstars: evolutionsupernovae: generalGalaxy: evolutionnuclear reactionsnucleosynthesis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 154 - 166
Copyright
Copyright © International Astronomical Union 2014 

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