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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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Nomoto et al. (1984) studied this question.
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