Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...223..244a&link_type=abstract
Astrophysical Journal, Part 1, vol. 223, July 1, 1978, p. 244-251.
Astronomy and Astrophysics
Astrophysics
101
Abundance, Computerized Simulation, Heavy Elements, Stellar Evolution, Stellar Mass, Galactic Evolution, Tables (Data)
Scientific paper
Stars of mass 2, 3, 5, 7, and 10 solar masses and chemical compositions (X = 0.7, Z = 0.03), (0.7,0.01), (0.7,0.003), (0.7,0.001), and (0.7,0.0004) have been evolved past core helium exhaustion (except for the 2-solar-mass stars, which are evolved to core helium ignition). These results demonstrate how the evolution of massive stars is determined by their initial heavy-element abundance and should be useful in the study of galactic evolution.
Alcock Charles
Paczyński Bohdan
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