Chemical yields from low- and intermediate-mass stars

Details Chemical yields from low- and intermediate-mass stars Chemical yields from low- and intermediate-mass stars

1999-12-16

arxiv.org/abs/astro-ph/9912341v1

Astronomy and Astrophysics

Astrophysics

6 pages, 4 postscript figures, to appear in "The chemical evolution of the Milky Way: stars versus clusters", Proceedings of t

Scientific paper

We present new sets of chemical yields from low- and intermediate-mass stars with 0.8 Msun <= M <= Mup ~ 5 Msun, and three choices of the metallicity, Z=0.02, Z=0.008, and Z=0.004 (Marigo 2000, in preparation). These are then compared with the yields calculated by other authors on the basis of different model prescriptions, and basic observational constraints which should be reproduced.

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