The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star-Reference-Cited by-同舟云学术

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

Published:2006-09 Issue:7109 Volume:443 Page:308-311
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Andrew Howell D.,Sullivan Mark,Nugent Peter E.,Ellis Richard S.,Conley Alexander J.,Le Borgne Damien,Carlberg Raymond G.,Guy Julien,Balam David,Basa Stephane,Fouchez Dominique,Hook Isobel M.,Hsiao Eric Y.,Neill James D.,Pain Reynald,Perrett Kathryn M.,Pritchet Christopher J.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature05103.pdf

Reference30 articles.

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3. Hoyle, F. & Fowler, W. A. Nucleosynthesis in supernovae. Astrophys. J. 132, 565–590 (1960)

4. Chandrasekhar, S. The maximum mass of ideal white dwarfs. Astrophys. J. 74, 81–82 (1931)

5. Sullivan, M. et al. Rates and properties of type Ia supernovae as a function of mass and star-formation in their host galaxies. Astrophys. J. (in the press); preprint at http://www.arXiv.org/astro-ph/0605455 (2006)

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