Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J-Reference-Cited by-同舟云学术

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Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J

Published:2014-08 Issue:7515 Volume:512 Page:406-408
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Churazov E.,Sunyaev R.,Isern J.,Knödlseder J.,Jean P.,Lebrun F.,Chugai N.,Grebenev S.,Bravo E.,Sazonov S.,Renaud M.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature13672.pdf

Reference43 articles.

1. Nomoto, K., Thielemann, F.-K. & Yokoi, K. Accreting white dwarf models of Type I supernovae. III - Carbon deflagration supernovae. Astrophys. J. 286, 644–658 (1984)

2. Woosley, S. E. & Weaver, T. A. The physics of supernova explosions. Annu. Rev. Astron. Astrophys. 24, 205–253 (1986)

3. Hillebrandt, W. & Niemeyer, J. C. Type Ia supernova explosion models. Annu. Rev. Astron. Astrophys. 38, 191–230 (2000)

4. Whelan, J. & Iben, I., Jr Binaries and supernovae of type I. Astrophys. J. 186, 1007–1014 (1973)

5. Iben, I., Jr & Tutukov, A. V. Supernovae of type I as end products of the evolution of binaries with components of moderate initial mass (M not greater than about 9 solar masses). Astrophys. J. Suppl. Ser. 54, 335–372 (1984)

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