KHz QPOs and their constraints on the pulsar parameters

Details KHz QPOs and their constraints on the pulsar parameters KHz QPOs and their constraints on the pulsar parameters

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..968..223z&link_type=abstract

ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP Conference Proceedings, Volum

Astronomy and Astrophysics

Astrophysics

1

Pulsars, Neutron Stars, X-Ray Binaries

Scientific paper

Khz QPO infers the millisecond oscillation close to the neutron star in the binary system. By means of the twin kHz QPOs, we can constrain the neutron star mass and radius. As the examples, we studied the sources Cir X-1, Cgy X-2, Sax J 1808.4-3658, XTE 1807-294 and the fastest nuclear-powered millisecond pulsar XTE J1739-285 with the spin frequency 1122 Hz.

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