Stellar models including pre-SN/SN phases

Details Stellar models including pre-SN/SN phases Stellar models including pre-SN/SN phases

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000newar..44..297h&link_type=abstract

New Astronomy Reviews, Volume 44, Issue 4-6, p. 297-302.

Astronomy and Astrophysics

Astronomy

5

Scientific paper

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 Msolar stars with different assumptions regarding the mixing efficiency of semiconvection and for rotating and non-rotating stellar models.

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