6533b7d1fe1ef96bd125c385

RESEARCH PRODUCT

Disc loss and renewal in A0535+26

M. J. CoeN. J. HaighJuan FabregatIain A. Steele

subject

PhysicsInfrared excessAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Infrared spectroscopyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSpace and Planetary ScienceIntermediate stateAstrophysics::Solar and Stellar AstrophysicsBinary systemAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsLine (formation)

description

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.

10.1046/j.1365-8711.1999.03148.xhttp://arxiv.org/abs/astro-ph/9910367