Progenitors of Type Ia Supernovae: Single Degenerate and Double Degenerates

Details Progenitors of Type Ia Supernovae: Single Degenerate and Double Degenerates Progenitors of Type Ia Supernovae: Single Degenerate and Double Degenerates

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1111..267n&link_type=abstract

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conferen

Computer Science

1

Supernova Remnants, Star Formation, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

We summarize some recent developments in theoretical studies on the progenitors of Type Ia supernovae (SNe Ia): (1) merging of double degenerates and associated off-center carbon ignition, (2) mass-stripping from the companion star by white dwarf winds, (3) the formation of circumstellar matter and the young population of SNe Ia, (4) delay time distribution in the single degenerate scenario, and (5) the origin of the transient heavy element absorption systems observed in novae.

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