A comparison of white dwarf mass estimators using the intermediate polar XY Ari

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 4, 1998, Pages 1269-1273

  Ramsay, Gavin ^a   Cropper, Mark ^a   Hellier, Coel ^b   Wu, Kinwah ^c  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b KEELE UNIVERSITY   (United Kingdom)

^c UNIVERSITY OF SYDNEY   (Australia)

Author keywords

Accretion, accretion discs; Novae, cataclysmic variables; Stars: individual: XY Ari; White dwarfs; X rays: stars

Indexed keywords

X RAY DETECTORS;

ACCRETION: ACCRETION DISKS; BEST FIT; BREMSSTRAHLUNG MODEL; INTERMEDIATE POLARS; NOVAE CATACLYSMIC VARIABLES; STAR: INDIVIDUAL: XY ARI; STARS: INDIVIDUAL: PROXIMA CENTAURI; X RAY ECLIPSE; X RAY SPECTRUM; X-RAY:STARS;

WHITE DWARFS;

EID: 0001077738     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01609.x     Document Type: Review

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