A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Substantial Disc Loss in the Be/X-ray Binary System A0535+26
2000
International Astronomical Union Colloquium
Preserved Fulltext
AbstractInfraredJHKphotometry from October 1998 revealed a remarkable change in the Be/X-ray binary system A0535+26, manifesting itself as a dramatic reduction in emission from the circumstellar disc. Optical and IR spectra presented here have confirmed this disc-loss in greater detail showing radically reduced Hydrogen and Helium line emission, to a degree never before seen in this system, and only rarely in a handful of Be/X-ray binaries. Optical spectroscopy has revealed the re-appearance of
doi:10.1017/s0252921100056864
fatcat:roj33pbc6vfo7hw2tursxu5yjm