The X-ray off-state of the supersoft source CAL 83 and its interpretation

Monthly Notices of the Royal Astronomical Society

Volumn 286, Issue 2, 1997, Pages 483-486

  Alcock, C ^a,b   Allsman, R A ^c   Alves, D ^a   Axelrod, T S ^a,d   Bennett, D P ^a,b   Charles, P A ^e   Cook, K H ^a,b   Freeman, K C ^d   Griest, K ^b,f   Guern, J ^b,f   Lehner, M J ^b,f   Livio, M ^g   Marshall, S L ^b,h   Peterson, B A ^d   Pratt, M R ^b,h   Quinn, P J ^d   Rodgers, A W ^d   Southwell, K A ^e   Stubbs, C W ^b,h,i   Sutherland, W ^e  

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^e UNIVERSITY OF OXFORD   (United Kingdom)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g STScI   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF WASHINGTON   (United States)

Author keywords

Accretion, accretion discs; Binaries: close; Binaries: spectroscopic; Stars: individual: CAL 83; X rays: atars

Indexed keywords

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BINARIES: SPECTROSCOPIC; OFF STATE; OPTICAL BEHAVIOUR; OPTICAL DATA; STAR: INDIVIDUAL: CAL 83; STARS: INDIVIDUAL: PROXIMA CENTAURI; TURN OFFS; X-RAY: ATARS;

WHITE DWARFS;

EID: 0009300352     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/286.2.483     Document Type: Article

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