Quasiperiodic oscillations in bright galactic-bulge X-ray sources

Details Quasiperiodic oscillations in bright galactic-bulge X-ray sources Quasiperiodic oscillations in bright galactic-bulge X-ray sources

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stin...8534723l&link_type=abstract

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Astronomy and Astrophysics

Astrophysics

Galactic Bulge, Neutron Stars, Stellar Oscillations, X Ray Astronomy, X Rays, Astrophysics, Earth Magnetosphere, Galactic Clusters, Galactic Radiation, Magnetic Stars

Scientific paper

Quasiperiodic oscillations with frequencies in the range 5-50 Hz have recently been discovered in X-rays from two bright galactic-bulge sources and Sco X-1. These sources are weakly magnetic neutron stars accreting from disks which the plasma is clumped. The interaction of the magnetosphere with clumps in the inner disk causes oscillations in the X-ray flux with many of the properties observed.

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