Be/X-ray binaries: An observational approach
Astrophysics
2009-03-24 v1
Abstract
Be/X-ray binaries are the most numerous class of X-ray binaries. They constitute an excellent tracer of star formation and can be used to study several aspects of astrophysics, from mass loss in massive stars to binary evolution. This short review, intended for the non-specialist, presents a summary of their basic observational properties and outlines the physical mechanisms giving rise to these characteristics.
Cite
@article{arxiv.astro-ph/0411335,
title = {Be/X-ray binaries: An observational approach},
author = {Ignacio Negueruela},
journal= {arXiv preprint arXiv:astro-ph/0411335},
year = {2009}
}
Comments
8 pages, 1 figure. Uses ASP Conference macro (included). Extended (mainly by expansion of the bibliography) version of short review appearing in Proceedings of "Massive Stars in Interacting Binaries" (Lac Sacacomie, Quebec, 16-20 Aug 2004) eds. N. St-Louis & A. Moffat, ASP Conf. Series