Slow neutron capture nucleosynthesis in the progenitor of SN 1987A

Details Slow neutron capture nucleosynthesis in the progenitor of SN 1987A Slow neutron capture nucleosynthesis in the progenitor of SN 1987A

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...331l..15p&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 331, Aug. 1, 1988, p. L15-L19.

Astronomy and Astrophysics

Astrophysics

16

Barium, Magellanic Clouds, Nuclear Astrophysics, Stellar Mass, Supernova 1987A, Thermal Neutrons, Abundance, Light Curve, Neutrino Beams, Nuclear Reactions

Scientific paper

The Ba overabundance detected in the SN 1987A ejecta (Williams, 1987;
Danziger et al., 1988) is intepreted in terms of slow-neutron-capture
nucleosynthesis during core He burning in the (presumed) progenitor
Sk-69 deg 202. The results of nucleosynthesis computations are reported,
and their relevance to the observations is discussed.

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