Stellar models including pre-SN/SN phases
Abstract
We present a grid of new models of rotating and non-rotating stars of solar metallicity. Their evolution was followed form the pre-main sequence stage up to core collapse using a 199 isotope network. The evolution and nucleosynthesis was continued through the supernova stage using a 'piston' model [Woosley, S.E, Weaver, T.A., 1995, ApJS, 101, 181] to simulate the explosion. Final isotopic yields are given for 15 and 25 M⊙ stars with different assumptions regarding the mixing efficiency of semiconvection and for rotating and non-rotating stellar models.
- Publication:
-
New Astronomy Reviews
- Pub Date:
- July 2000
- DOI:
- 10.1016/S1387-6473(00)00043-9
- Bibcode:
- 2000NewAR..44..297H