Chemical yields from low- and intermediate-mass stars
arXiv:astro-ph/9912341 · doi:10.1007/978-94-010-0938-6_47
Abstract
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.
6 pages, 4 postscript figures, to appear in "The chemical evolution of the Milky Way: stars versus clusters", Proceedings of the Roma-Trieste Workshop, (Vulcano, September 1999), eds. F. Matteucci and F. Giovannelli