Type Ia Supernovae: Progenitors and Peculiarity

dc.contributor.author	Nomoto, K
dc.contributor.author	Tanaka, M
dc.contributor.author	Kawabata, K. S
dc.contributor.author	Sahu, D. K
dc.contributor.author	Anupama, G. C
dc.date.accessioned	2011-09-22T14:47:24Z
dc.date.available	2011-09-22T14:47:24Z
dc.date.issued	2007-08
dc.identifier.citation	AIP Conference Proceedings, Vol. 924, pp. 194-202	en
dc.identifier.uri	http://hdl.handle.net/2248/5575
dc.description.abstract	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	en
dc.language.iso	en	en
dc.publisher	American Institute of Physics	en
dc.relation.uri	http://link.aip.org/link/?APCPCS/924/194/1	en
dc.rights	© American Institute of Physics	en
dc.subject	Supernovae	en
dc.subject	Faint blue stars	en
dc.subject	White dwarfs	en
dc.subject	Stellar structure	en
dc.title	Type Ia Supernovae: Progenitors and Peculiarity	en
dc.type	Article	en