Type Ia Supernovae: Progenitors and Peculiarity

Details Type Ia Supernovae: Progenitors and Peculiarity Type Ia Supernovae: Progenitors and Peculiarity

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..924..194n&link_type=abstract

THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. AIP Conference Proceedings, Volume 924, pp. 194-202

Computer Science

Supernovae, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

Among the controversial issues on Type Ia supernovae (SNe Ia), we discuss (1) the evolutionary paths of the progenitor systems to SNe Ia, especially, the thermal stability of hydrogen shell burning in accreting white dwarfs, and (2) SN 2005hk which belongs to the very peculiar 2002cx-like group of SNe Ia. For SN 2005hk, we show our observations of the light curve and late time spectra, and present a preliminary model for the light curve to confirm it is quite a low energy explosion.

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