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Laboratory analogue of a supersonic accretion column in a binary star system

Authors :
J. E. Cross
G. Gregori
J. M. Foster
P. Graham
J. -M. Bonnet-Bidaud
C. Busschaert
N. Charpentier
C. N. Danson
H. W. Doyle
R. P. Drake
J. Fyrth
E. T. Gumbrell
M. Koenig
C. Krauland
C. C. Kuranz
B. Loupias
C. Michaut
M. Mouchet
S. Patankar
J. Skidmore
C. Spindloe
E. R. Tubman
N. Woolsey
R. Yurchak
É. Falize
Source :
Nature Communications, Vol 7, Iss 1, Pp 1-7 (2016)
Publication Year :
2016
Publisher :
Nature Portfolio, 2016.

Abstract

Stationary radiative shocks are expected to form above the surface of highly-magnetized white dwarves in binary systems, but this cannot be resolved by telescopes. Here, the authors report a laboratory experiment showing the evolution of a reverse shock when both ionization and radiative losses are important.

Subjects

Subjects :
Science

Details

Language :
English
ISSN :
20411723
Volume :
7
Issue :
1
Database :
Directory of Open Access Journals
Journal :
Nature Communications
Publication Type :
Academic Journal
Accession number :
edsdoj.7e067a3843f4aaa843c5594b4089ab6
Document Type :
article
Full Text :
https://doi.org/10.1038/ncomms11899