Evolution, Explosion, and Nucleosynthesis of Core‐Collapse Supernovae

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 20 Jul 2003Embargo end date: 01 Jan 2003 Australia, Italy, Italy English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 592, pages 404-433 (issn: 0004-637X, eissn: 1538-4357,

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Authors: Limongi, Marco; Chieffi, Alessandro;

doi: 10.1086/375703 , 10.48550/arxiv.astro-ph/0304185 , 10.25916/sut.26289007.v1 , 10.25916/sut.26289007

arXiv: astro-ph/0304185

handle: 1959.3/1181

Evolution, Explosion, and Nucleosynthesis of Core‐Collapse Supernovae

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Abstract

We present a new set of presupernova evolutions and explosive yields of massive stars of initial solar composition (Y=0.285, Z=0.02) in the mass range 13-35 Msun. All the models have been computed with the latest version (4.97) of the FRANEC code that now includes a nuclear network extending from neutrons to Mo98. The explosive nucleosynthesis has been computed twice: a first one with an hydro code and a second one following the simpler radiation dominated shock approximation (RDA).

20 pages, 10 figures, 12 tables. Accepted for publication on ApJ

Countries

Australia, Italy, Italy

Related Organizations

Osservatorio di Astrofisica e Scienza dello Spazio
Italy
National Institute for Astrophysics
Italy
Swinburne University of Technology
Australia
National Research Council
Italy
National Institute for Nuclear Physics
Italy

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Keywords

NEANIAS Space Research Community, Space and Planetary Science, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, 520

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