Explosive nucleosynthesis and Type I supernovae

Details Explosive nucleosynthesis and Type I supernovae Explosive nucleosynthesis and Type I supernovae

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...279l..23n&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 279, April 1, 1984, p. L23-L26. Research supported

Astronomy and Astrophysics

Astrophysics

48

Nuclear Fusion, Supermassive Stars, Supernovae, Abundance, Carbon Stars, White Dwarf Stars

Scientific paper

The ejecta of a particular carbon deflagration model for Type I supernovae are combined with the ejecta of a massive star to show that Type I supernovae may be important contributors to galactic nucleosynthesis. Type I supernovae may help to fill in the paucity of oxygen-burning products from the massive stars. Problems with the overproduction of 16O from massive stars and 40Ca, 56Fe, and 54Fe from deflagration models of Type I supernovae are discussed.

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