Lower bounds on neutron star radii from measurements of the x-ray spectra of low-mass x-ray binaries

Details Lower bounds on neutron star radii from measurements of the x-ray spectra of low-mass x-ray binaries Lower bounds on neutron star radii from measurements of the x-ray spectra of low-mass x-ray binaries

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..409k&link_type=abstract

Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astrophysics

Neutron Stars, X-Ray Binaries, Stellar Characteristics And Properties

Scientific paper

Recently discovered correlations between variations in the x-ray spectrum and the frequency of fast quasiperiodic oscillations from the neutron star x-ray binary 4U 0614+091 suggest that a soft blackbody component of the x-ray spectrum arises from the accretion disk. Here, we show that this identification, if correct, may allow one to obtain lower bounds on the radii of neutron stars from measurements of their x-ray spectra.

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