Abstract
view Abstract Citations (105) References (17) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The effect of the heavy element abundance on the evolution of stars. Alcock, C. ; Paczynski, B. Abstract 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. Publication: The Astrophysical Journal Pub Date: July 1978 DOI: 10.1086/156256 Bibcode: 1978ApJ...223..244A Keywords: Abundance; Computerized Simulation; Heavy Elements; Stellar Evolution; Stellar Mass; Galactic Evolution; Tables (Data); Astrophysics; Element Abundances:Stellar Evolution full text sources ADS |
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