Pulsar Mass and Radius Estimation by the Khz QPO

Details Pulsar Mass and Radius Estimation by the Khz QPO Pulsar Mass and Radius Estimation by the Khz QPO

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010gras.conf..309z&link_type=abstract

GRAVITATION AND ASTROPHYSICS. Proceedings of the Ninth Asia-Pacific International Conference. Held 29 June-2 July 2009 in Wuhan,

Astronomy and Astrophysics

Astrophysics

Pulsar, Khz Qpos, Binary System

Scientific paper

RXTE satellite discovered many kHz quasi-periodic oscillations (QPOs) in X-ray neuron star systems, and these oscillations are often taken as the accreting matter circling around the central compact objects. As the models for kHz QPOs are constructed, the mass and/or radius of these neutron stars can be inferred, by which the comparisons with the star equations of states (EOSs) can be performed.

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