Long-term variability of the Be/X-ray binary A0535+26 - III. Photometry

Monthly Notices of the Royal Astronomical Society

Volumn 302, Issue 1, 1999, Pages 167-172

  Clark, J S ^a,b   Lyuty, V M ^f   Zaitseva, G V ^f   Larionov, V M ^c   Larionova, L V ^c   Finger, M ^d   Tarasov, A E ^e   Roche, P ^a   Coe, M J ^b  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^d NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^e CRIMEAN ASTROPHYSICAL OBSERVATORY   (Ukraine)

^f NONE

Author keywords

Accretion, accretion discs; Binaries: close; Circumstellar matter; Stars: emission line, Be; Stars: individual: A0535+26; X rays: stars

Indexed keywords

OPTICAL CORRELATION; PHOTOMETRY;

ACCRETION: ACCRETION DISKS; BE-X-RAYS:BINARIES; BINARIES: CLOSE; CIRCUMSTELLAR MATTERS; LIGHT CURVES; MASS LOSS RATE; STAR: INDIVIDUAL: A0535+26; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY:STARS;

STARS;

EID: 0001374124     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02112.x     Document Type: Article

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