On the nonpulsation of QPOs and Galactic bulge neutron star X-ray sources

Details On the nonpulsation of QPOs and Galactic bulge neutron star X-ray sources On the nonpulsation of QPOs and Galactic bulge neutron star X-ray sources

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...325..204m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 325, Feb. 1, 1988, p. 204-206.

Astronomy and Astrophysics

Astrophysics

21

Galactic Bulge, Magnetic Stars, Neutron Stars, Relativity, Stellar Oscillations, X Ray Binaries

Scientific paper

It is shown that general-relativistic (GR) light bending is extremely
efficient in reducing below 1 percent the pulsed fraction of low
magnetic field, small radius neutron stars. Such stars may be present in
QPOs and Galactic bulge X-ray sources.

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