X-ray observations of 4 Draconis: Symbiotic binary or cataclysmic triple?

Monthly Notices of the Royal Astronomical Society

Volumn 346, Issue 3, 2003, Pages 855-860

  Wheatley, Peter J ^a   Mukai, Koji ^b,d   De Martino, Domitilla ^c  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^d UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

Author keywords

Accretion, accretion discs; Binaries: close; Novae, cataclysmic variables; Stars: individual: 4 Draconis; White dwarfs; X rays: stars

Indexed keywords

ABSORPTION SPECTROSCOPY; GIANT STARS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BINARY SYSTEMS; CATACLYSMIC VARIABLES; NOVAE CATACLYSMIC VARIABLES; STAR: INDIVIDUAL: 4 DRACONIS; STARS: INDIVIDUAL: PROXIMA CENTAURI; SYMBIOTICS; X-RAY OBSERVATIONS; X-RAY:STARS;

WHITE DWARFS;

EID: 0348158212     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2003.07149.x     Document Type: Article

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