Be stars in X-ray binary systems

M. J. Coe

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arXiv · astro-ph/9911272

Be stars in X-ray binary systems

M. J. Coe

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Abstract

This paper will review the status of our observations and understanding of Be stars in X-ray binary systems. In virtually all cases the binary partner to the Be star is a neutron star. The circumstellar disk provides the accretion fuel and hence stimulates the X-ray emission, whilst the neutron star provides a valuable probe of the environment around the Be star. The results coming from studies of such systems are helping in our understanding of the Be phenomenon.

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M. J. Coe. 1999-11-15. Be stars in X-ray binary systems. https://arxiv.org/abs/astro-ph/9911272

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