The Be/X-ray transient V0332+53: Evidence for a tilt between the orbit and the equatorial plane?

Monthly Notices of the Royal Astronomical Society

Volumn 307, Issue 3, 1999, Pages 695-702

  Negueruela, I ^a,b   Roche, P ^c   Fabregat, J ^d   Coe, M J ^e  

^a LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^b BeppoSAX Science Data Center   (Italy)

^c UNIVERSITY OF SUSSEX   (United Kingdom)

^d UNIVERSITY OF VALENCIA   (Spain)

^e UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Binaries: general; BQ Cam; Infrared: stars; Pulsars: general; Stars: emission line, Be; Stars: individual; X rays: stars

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; PULSARS;

BINARIES:GENERAL; BQ CAM; CIRCUMSTELLAR DISKS; EQUATORIAL PLANES; INFRARED: STAR; PULSARS: GENERAL; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY TRANSIENTS; X-RAY:STARS;

CAMS;

EID: 0008541393     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02682.x     Document Type: Article

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