X-ray beaming caused by resonance scattering in the accretion column of magnetic cataclysmic variables

Monthly Notices of the Royal Astronomical Society

Volumn 328, Issue 1, 2001, Pages 112-126

  Terada, Y ^a   Ishida, M ^b   Makishima, K ^a   Imanari, T ^a   Fujimoto, R ^c   Matsuzaki, K ^c   Kaneda, H ^c  

^a UNIVERSITY OF TOKYO   (Japan)

^b TOKYO METROPOLITAN UNIVERSITY   (Japan)

^c JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

Author keywords

Methods: observational; Radiation mechanisms: thermal; Scattering; Stars: individual: V834 Cen; White dwarfs; X rays: stars

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; INTELLIGENT SYSTEMS; IRON; MONTE CARLO METHODS; PHOTONS;

CATACLYSMIC VARIABLES; COMPACT OBJECTS; EMISSION LINES; EQUIVALENT WIDTH; METHODS:OBSERVATIONAL; RADIATION MECHANISM: THERMAL; RESONANCE SCATTERING; STAR: INDIVIDUAL: V834 CEN; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY:STARS;

WHITE DWARFS;

EID: 0042869774     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04878.x     Document Type: Article

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