Binary orbits as the driver of γ-ray emission and mass ejection in classical novae-Reference-Cited by-同舟云学术

Binary orbits as the driver of γ-ray emission and mass ejection in classical novae

Published:2014-10 Issue:7522 Volume:514 Page:339-342
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Chomiuk Laura,Linford Justin D.,Yang Jun,O’Brien T. J.,Paragi Zsolt,Mioduszewski Amy J.,Beswick R. J.,Cheung C. C.,Mukai Koji,Nelson Thomas,Ribeiro Valério A. R. M.,Rupen Michael P.,Sokoloski J. L.,Weston Jennifer,Zheng Yong,Bode Michael F.,Eyres Stewart,Roy Nirupam,Taylor Gregory B.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature13773.pdf

Reference38 articles.

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2. Starrfield, S., Truran, J. W., Sparks, W. M. & Kutter, G. S. CNO abundances and hydrodynamic models of the nova outburst. Astrophys. J. 176, 169–176 (1972)

3. Kato, M. & Hachisu, I. Optically thick winds in nova outbursts. Astrophys. J. 437, 802–826 (1994)

4. MacDonald, J. The effect of a binary companion on a nova outburst. Mon. Not. R. Astron. Soc. 191, 933–949 (1980)

5. The Fermi-LAT collaboration. Fermi establishes classical novae as a distinct class of γ-ray sources. Science 345, 554–558 (2014)

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