Condensation in Supernova Ejecta at High Spatial Resolution

Computer Science

Scientific paper

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Scientific paper

^44Ti-rich TiC condenses before graphite in SN ejecta only if thin
sub-layers of the main burning zones mix together; such mixing is also
needed to form Fe-olivine. High-T phases change from carbides to oxides
along composition gradients within the He/N zone.

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