Interaction of accretion disk and rotating magnetic field of neutron star

Details Interaction of accretion disk and rotating magnetic field of neutron star Interaction of accretion disk and rotating magnetic field of neutron star

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979esasp.148..263a&link_type=abstract

In ESA Magnetospheric Boundary Layers p 263-264 (SEE N80-13529 04-42)

Physics

Neutron Stars, Stellar Magnetic Fields, Stellar Mass Accretion, Boundary Layer Stability, Gas Flow, Stellar Models, Turbulent Diffusion, X Ray Sources

Scientific paper

Utilizing the instabilities of the boundary between disk and magnetosphere, a model for the flow of disk material into the neutron star's magnetosphere is constructed. It is shown that within a thin ring around the corotation radius, gas flows over. The gas is partly accelerated towards the neutron star producing the accretion partly outwards. In terms of this model, certain observed properties of pulsating X-ray sources are explained.

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