Open AccessA Steady State Model of X-Ray Emitting Coronae around Accreting Non-Magnetic White Dwarfs in Cataclysmic Variables
Author(s) -
P. Mahasena,
Yoji Osaki
Publication year - 1999
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/51.1.45
Subject(s) - physics , white dwarf , astrophysics , accretion (finance) , intermediate polar , cataclysmic variable star , dwarf nova , eclipse , corona (planetary geology) , light curve , astronomy , stars , astrobiology , venus
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