On the nature of the X-ray source in GK Persei

Astronomy and Astrophysics

Volumn 439, Issue 1, 2005, Pages 287-300

  Vrielmann, S ^a   Ness, J U ^b   Schmitt, J H M M ^a  

^a UNIVERSITY OF HAMBURG   (Germany)

^b UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Accretion, accretion disks; Stars: binaries: close; Stars: individual: GK Per; Stars: novae, cataclysmic variables; X rays: stars

Indexed keywords

CARRIER CONCENTRATION; ELECTRONS; MAGNETIZATION; SCATTERING; ULTRAVIOLET RADIATION; X RAYS;

ACCRETION DISKS; CATACLYSMIC VARIABLES; STARS: BINARIES: CLOSE; STARS: INDIVIDUAL: GK PER; STARS: NOVAE; X-RAY: STARS;

ASTROPHYSICS;

EID: 23844523545     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053017     Document Type: Article

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