Constraining type Ia supernovae progenitors from three years of supernova legacy survey data

Constraining type Ia supernovae progenitors from three years of supernova legacy survey data

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While it is generally accepted that Type Ia supernovae are the result of the explosion of a carbon-oxygen white dwarf accreting mass in a binary system, the details of their genesis still elude us, and the nature of the binary companion is uncertain. Kasen points out that the presence of a non-degen...

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Bibliographic Details
Main Authors: Bianco, F, Howell, D, Sullivan, M, Conley, A, Kasen, D, Gonzlez-Gaitn, S, Guy, J, Astier, P, Balland, C, Carlberg, R, Fouchez, D, Fourmanoit, N, Hardin, D, Hook, I, Lidman, C, Pain, R, Palanque-Delabrouille, N, Perlmutter, S, Perrett, K, Pritchet, C, Regnault, N, Rich, J, Ruhlmann-Kleider, V
Format: Journal article
Language:English
Published: 2011

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