Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...264..278b&link_type=abstract
Astrophysical Journal, Part 1, vol. 264, Jan. 1, 1983, p. 278-281. Research supported by the Natural Sciences and Engineering R
Astronomy and Astrophysics
Astrophysics
1
Ground State, Nuclear Fusion, Reaction Kinetics, Stars, Calcium, Oxygen, Silicon, Stellar Mass, Stellar Temperature
Scientific paper
Ground-state reaction rates have been deduced from recent cross section measurements for the 39K(α, p)42Ca, 42Ca(α, p)45Sc, 42Ca(α, n)45Ti, 42Ca(p, γ)43Sc, and 44Ca(p, n)44Sc reactions. Stellar reaction rates have been derived from the ground-state rates by multiplying by the ratio of stellar to ground-state rates obtained from statistical model calculations. Stellar rates for the four exoergic reverse reactions have been derived using the procedures of Woosley et al.
Buckby Margaret Anna Maria
King J. D.
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