Supernova SN 2011fe from an exploding carbon–oxygen white dwarf star-Reference-Cited by-同舟云学术

Supernova SN 2011fe from an exploding carbon–oxygen white dwarf star

Published:2011-12 Issue:7377 Volume:480 Page:344-347
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Nugent Peter E.,Sullivan Mark,Cenko S. Bradley,Thomas Rollin C.,Kasen Daniel,Howell D. Andrew,Bersier David,Bloom Joshua S.,Kulkarni S. R.,Kandrashoff Michael T.,Filippenko Alexei V.,Silverman Jeffrey M.,Marcy Geoffrey W.,Howard Andrew W.,Isaacson Howard T.,Maguire Kate,Suzuki Nao,Tarlton James E.,Pan Yen-Chen,Bildsten Lars,Fulton Benjamin J.,Parrent Jerod T.,Sand David,Podsiadlowski Philipp,Bianco Federica B.,Dilday Benjamin,Graham Melissa L.,Lyman Joe,James Phil,Kasliwal Mansi M.,Law Nicholas M.,Quimby Robert M.,Hook Isobel M.,Walker Emma S.,Mazzali Paolo,Pian Elena,Ofek Eran O.,Gal-Yam Avishay,Poznanski Dovi

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature10644.pdf

Reference27 articles.

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3. Sullivan, M. et al. SNLS3: constraints on dark energy combining the supernova legacy survey three-year data with other probes. Astrophys. J. 737, 102–121 (2011)

4. Howell, D. A. Type Ia supernovae as stellar endpoints and cosmological tools. Nature Commun. 2, 350 (2011)

5. Kasen, D., Röpke, F. K. & Woosley, S. E. The diversity of type Ia supernovae from broken symmetries. Nature 460, 869–872 (2009)

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