The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star.

The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that have accreted matter from a companion star, alt...

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Detalles Bibliográficos
Autores principales:	Howell, D, Sullivan, M, Nugent, P, Ellis, R, Conley, A, Le Borgne, D, Carlberg, R, Guy, J, Balam, D, Basa, S, Fouchez, D, Hook, I, Hsiao, E, Neill, J, Pain, R, Perrett, K, Pritchet, C
Formato:	Journal article
Lenguaje:	English
Publicado:	2006

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star por Howell, D, Sullivan, M, Nugent, P, Ellis, R, Conley, A, Le Borgne, D, Carlberg, R, Guy, J, Balam, D, Basa, S, Fouchez, D, Hook, I, Hsiao, E, Neill, J, Pain, R, Perrett, K, Pritchet, C

Publicado 2006

Journal article

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star.

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star por Howell, D, Sullivan, M, Nugent, P, Ellis, R, Conley, A, Le Borgne, D, Carlberg, R, Guy, J, Balam, D, Basa, S, Fouchez, D, Hook, I, Hsiao, E, Neill, J, Pain, R, Perrett, K, Pritchet, C

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