Explosive yields of massive stars from Z=0 to Z=Zsun

Details Explosive yields of massive stars from Z=0 to Z=Zsun Explosive yields of massive stars from Z=0 to Z=Zsun

2004-02-26

arxiv.org/abs/astro-ph/0402625v1

Astrophys.J. 608 (2004) 405-410

Astronomy and Astrophysics

Astrophysics

Accepted for publication on The Astrophysical Journal. 41 pages, 3 figures, 1 Table

Scientific paper

10.1086/392523

We present a new and homogeneous set of explosive yields for masses 13, 15, 20, 25, 30 and 35 Msun and metallicities Z=0, 10^{- 6}, 10^{- 4}, 10^{- 3}, 6x10^{- 3}, 2x10^{-2}. A wide network extending up to Mo has been used in all the computation. 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 that 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 upon request.

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