Be/X-ray binaries: An observational approach

Details Be/X-ray binaries: An observational approach Be/X-ray binaries: An observational approach

2004-11-12

arxiv.org/abs/astro-ph/0411335v1

ASP Conf.Ser.367:477,2007

Astronomy and Astrophysics

Astrophysics

8 pages, 1 figure. Uses ASP Conference macro (included). Extended (mainly by expansion of the bibliography) version of short r

Scientific paper

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.

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