Neutron capture nucleosynthesis and the evolution of 15 and 30 solar-mass stars. I - The core helium burning phase

Details Neutron capture nucleosynthesis and the evolution of 15 and 30 solar-mass stars. I - The core helium burning phase Neutron capture nucleosynthesis and the evolution of 15 and 30 solar-mass stars. I - The core helium burning phase

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...210..187l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 210, no. 1-2, Feb. 1989, p. 187-197.

Astronomy and Astrophysics

Astrophysics

38

Neutrons, Nuclear Capture, Nuclear Fusion, Stellar Evolution, Stellar Mass, Supergiant Stars, Carbon Monoxide, Helium, Stellar Cores, Stellar Models, Temperature Dependence

Scientific paper

Neutron capture nucleosynthesis during central He-burning in massive (M/ZAMS/ = 15 and 30 solar-mass stars) mass-losing population I stars with and without convective overshooting, is studied by coupling a stellar evolution code to a detailed nucleosynthesis network. The nucleosynthesis is followed with the aid of a full reaction network incorporating up-to-date Maxwellian averaged neutron capture cross-sections, and new density- and temperature-dependent beta-decay and electron capture rates.

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