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We describe kHz QPOs from the hydrodynamical model of accretion disks forLMXB systems. Out of the pair, the higher frequency originates due to theviscous effects of an accretion disk involving the formation of shock, whilethe lower one is due to the Keplerian motion of accreting matter. Comparing ourresults with observations for two fast rotating compact stellar candidates,namely, 4U 1636-53 and KS 1731-260, we find that they match to a very goodapproximation.Comment: 3 latex pages including 1 figure; to appear in the proceedings of X  Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July 2003; on the basis of  talk presente

THEORETICAL DESCRIPTION OF KHZ QPOS IN ACCRETING LMXB SYSTEMS