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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5575
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dc.contributor.authorNomoto, K-
dc.contributor.authorTanaka, M-
dc.contributor.authorKawabata, K. S-
dc.contributor.authorSahu, D. K-
dc.contributor.authorAnupama, G. C-
dc.date.accessioned2011-09-22T14:47:24Z-
dc.date.available2011-09-22T14:47:24Z-
dc.date.issued2007-08-
dc.identifier.citationAIP Conference Proceedings, Vol. 924, pp. 194-202en
dc.identifier.urihttp://hdl.handle.net/2248/5575-
dc.description.abstractAmong 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 explosionen
dc.language.isoenen
dc.publisherAmerican Institute of Physicsen
dc.relation.urihttp://link.aip.org/link/?APCPCS/924/194/1en
dc.rights© American Institute of Physicsen
dc.subjectSupernovaeen
dc.subjectFaint blue starsen
dc.subjectWhite dwarfsen
dc.subjectStellar structureen
dc.titleType Ia Supernovae: Progenitors and Peculiarityen
dc.typeArticleen
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