Advances in Space Research, Volume 38, Issue 12, p. 2731-2736.
Bibcode
Casares, J.; Charles, Phil
Bibliographical reference
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2006
Journal
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Description
The determination of fundamental parameters in X-ray luminous
(persistent) X-ray binaries has been classically hampered by the large
optical luminosity of the accretion disc. New methods, based on
irradiation of the donor star and burst oscillations, provide the
opportunity to derive dynamical information and mass constraints in many
persistent systems for the first time. These techniques are here
reviewed and the latest results presented.