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A procedure which is relatively insensitive to the details of galactic evolutionary models is used to examine the production of iron-group nuclei to be expected from the carbon-detonation supernova model. The requirement that iron production be such as to reproduce the observed Fe/(C + 0) abundance ratio places severe constraints on either (1) the frequency of such events or (2) the amount of iron-group elements ejected from such an event. Subject headings: abundances, stellar - nucleosynthesis - stellar evolution - supernovae
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W. David Arnett (1974) studied this question.
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