How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy,General Biochemistry, Genetics and Molecular Biology,General Chemistry
Link
http://www.nature.com/articles/s41467-018-03548-7.pdf
Reference18 articles.
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2. Nymark, T. K., Fransson, C. & Kozma, C. X-ray emission from radiative shocks in type II supernovae. Astron. Astrophys. 449, 171–192 (2006).
3. Chevalier, R. A. The interaction of the radiation from a Type II supernova with a circumstellar shell. Astrophys. J. 251, 259–265 (1981).
4. Ensman, L. & Burrows, A. Shock breakout in SN1987A. Astrophys. J. 393, 742–755 (1992).
5. Tolstov, A., Blinnikov, S. I. & Nadyozhin, D. K. Coupling of matter and radiation at supernova shock breakout. Mon. Not. R. Astron. Soc. 429, 3181–3199 (2013).
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