Explosive Yields of Massive Stars fromZ= 0 toZ=Z⊙

2004/02/26 by A. Chieffi, Alessandro Chieffi, Marco Limongi · 25 citations
Physics and Astronomy · #Astro and Planetary Science #Gamma-ray bursts and supernovae #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1086/392523

published as Astrophys.J. 608 (2004) 405-410 · Accepted for publication on The Astrophysical Journal. 41 pages, 3 figures, 1 Table

arxiv created 2004/02/26 · openalex publication_date 2004/06/07 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We present a new and homogeneous set of explosive yields for masses 13, 15, 20, 25, 30, and 35 M ☉ and metallicities Z = 0, 10 -6 , 10 -4 , 10 -3 , 6 × 10 -3 , and 2 × 10 -2 . A wide network extending up to Mo has been used in all computations. We show that at low metallicities ( Z ≤ 10 -4 ), the final yields do not depend significantly on the initial chemical composition of the models, so a scaled solar distribution may be safely assumed at all metallicities. Moreover, no elements above Zn are produced by any mass in the grid up to a metallicity ~10 -3 . These yields are available for any choice of the mass cut on request.

Citations

• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis

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