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Restrictions to neutron star models based on twin-peak quasi-periodic oscillations
Published online by Cambridge University Press: 20 March 2013
Abstract
In a series of works - Török et al. (2010, 2012a) and Urbanec et al. (2010a) - we explored restrictions to neutron star properties that are implied by various models of twin-peak quasi-periodic oscillations. Here we sketch an attempt to confront the obtained mass–angular-momentum relations and limits on neutron star compactness with the parameters estimated by assuming various equations of state and the spin frequency of the atoll source 4U 1636-53.
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- Copyright © International Astronomical Union 2013