A steady state model of x-ray emitting coronae around accreting non-magnetic white dwarfs in cataclysmic variables

Publications of the Astronomical Society of Japan

Volumn 51, Issue 1, 1999, Pages 45-52

  Mahasena, Putra ^a,b   Osaki, Yoji ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b BANDUNG INSTITUTE OF TECHNOLOGY   (Indonesia)

Author keywords

Accretion; Stars: Cataclysmic; Stars: Coronae; Stars: Dwarf novae; X rays: Spectra

Indexed keywords

BOUNDARY LAYERS;

ACCRETION; CATACLYSMIC VARIABLES; MAGNETIC WHITE DWARFS; NONMAGNETICS; STARS: CORONA; STARS: DWARF NOVAE; STARS:CATACLYSMIC; STEADY-STATE MODELS; X RAY SPECTRUM; X-RAY EMITTING;

WHITE DWARFS;

EID: 0033244794     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/51.1.45     Document Type: Article

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