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Parameter constrain in neutron star by twin kHz QPOs

Published online by Cambridge University Press:  21 February 2013

D. H. Wang  and
L. Chen
D. H. Wang
Affiliation:
Astronomy Department, Beijing Normal University, Beijing 100875, China email: huazai05105220@163.com
L. Chen
Affiliation:
Astronomy Department, Beijing Normal University, Beijing 100875, China email: huazai05105220@163.com
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Abstract

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We use data on twin kHz QPOs and measured neutron star (NS) masses to test the relation between the lower (ν1) and upper (ν2) peak frequencies predicted with the MHD Alfvén wave oscillation model (AWOM) and the general relativistic precession model (GRPM). In the context of AWOM, the NS radius can be constrained from kHz QPO data and a measured NS mass.

Keywords

X-rays: binariesstars: neutronaccretionaccretion disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 325 - 326
Copyright
Copyright © International Astronomical Union 2013

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