Disc loss and renewal in A0535+26N.J.Haigh1, M.J.Coe1, I.A.Steele2, and J.Fabregat3
1
Department of Physics and Astronomy, The University, Southampton,
SO17 1BJ, UK
This paper presents observations of the Be/X-ray binary system A0535+26 revealing the first observed loss of its circumstellar disc, demonstrated by the loss of its JHK infrared excess and optical/IR line emission. However optical/IR spectroscopy reveals the formation of a new inner disc with significant density and emission strength at small radii; the disc has proven to be stable over 5 months in this intermediate state. 1999, MNRAS, 310, 21 |
Last modified: June 13, 2000
David McDavid