Evolution, Explosion, and Nucleosynthesis of Core‐Collapse Supernovae
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- 20 July 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 592 (1) , 404-433
- https://doi.org/10.1086/375703
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).Comment: 20 pages, 10 figures, 12 tables. Accepted for publication on ApKeywords
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