Abstract
This discussion will be highly circumscribed in a few respects. First, I shall limit my attention to those compact galactic X-ray sources whose X-ray luminosities are considerably in excess of the solar luminosity, and in particular I shall exclude from my discussion the weak X-ray emission that has been detected from many apparently isolated stars (Linsky 1980; Vaiana 1980). I shall also exclude any detailed discussion of individual peculiar objects and shall instead concentrate on the general trends among the majority of the bright galactic sources.
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Joss, P.C. (1981). Models for Galactic X-Ray Sources. In: Giacconi, R. (eds) X-Ray Astronomy with the Einstein Satellite. Astrophysics and Space Science Library, vol 87. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-8459-2_7
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