Computer Science
Scientific paper
Mar 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..241g&link_type=abstract
FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 241-243 (2008).
Computer Science
Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Supernovae, Population Iii Stars, Mass Loss And Stellar Winds, Giant And Subgiant Stars
Scientific paper
We have computed and analyzed the evolution of primordial stars of ZAMS masses between 5 and 10 Msolar, with and without overshooting, up to the early TP-(S) AGB. The initial mass limits for the formation of carbon-oxygen, oxygen-neon degenerate cores and core-collapse supernovae after the main central burning stages have been determined. The possible final fates of the considered stars have been explored in the frame of the existing uncertainties.
Garcia-Berro Enrique
Gil-Pon Pilar
Gutierrez Jordi
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