Open AccessThe Be/X‐ray transient V0332+53: evidence for a tilt between the orbit and the equatorial plane?
Author(s) -
Negueruela I.,
Roche P.,
Fabregat J.,
Coe M. J.
Publication year - 1999
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1999.02682.x
Subject(s) - physics , tilt (camera) , x ray transient , orbit (dynamics) , transient (computer programming) , plane (geometry) , astronomy , astrophysics , orbital plane , x ray , optics , geometry , neutron star , aerospace engineering , mathematics , computer science , engineering , operating system
We present optical and infrared observations of BQ Cam, the optical counterpart to the Be/X‐ray transient system V0332+53. BQ Cam is shown to be an O8–9Ve star, which places V0332+53 at a distance of ∼7 kpc. H α spectroscopy and infrared photometry are used to discuss the evolution of the circumstellar envelope. Owing to the low inclination of the system, parameters are strongly constrained. We find strong evidence for a tilt of the orbital plane with respect to the circumstellar disc (presumably on the equatorial plane). Even though the periastron distance is only ≈10 R * , during the present quiescent state the circumstellar disc does not extend to the distance of periastron passage. Under these conditions, X‐ray emission is effectively prevented by centrifugal inhibition of accretion. The circumstellar disc is shown to be optically thick at optical and infrared wavelengths, which, together with its small size, is taken as an indication of tidal truncation.