We present a Resonant Switch (RS) model of twin peak high-frequency
quasi-periodic oscillations (HF QPOs), assuming switch of twin oscillations at
a resonant point, where frequencies of the upper and lower oscillations νU
and νL become to be commensurable and the twin oscillations change from
one pair of the oscillating modes (corresponding to a specific model of HF
QPOs) to some other pair due to non-linear resonant phenomena. The RS model
enables to determine range of allowed values of spin a and mass M of the
neutron star located at the atoll source 4U 1636-53 where two resonant points
are observed at frequency ratios νU:νL = 3:2, 5:4.Comment: 2 pages, to be published in Proceedings of IAUS 290 "Feeding Compact
Objects: Accretion on All Scales", C. M. Zhang, T. Belloni, M. Mendez and S.
N. Zhang (eds.