Current diversion in the accretion disk of a magnetized neutron star

Details Current diversion in the accretion disk of a magnetized neutron star Current diversion in the accretion disk of a magnetized neutron star

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ncimc..12..113m&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 12 C, Jan.-Feb. 1989, p. 113-115. Research supported by Korea Institute of Techn

Physics

Accretion Disks, Magnetic Stars, Magnetohydrodynamic Flow, Neutron Stars, Lines Of Force, Stellar Magnetospheres, Stellar Models

Scientific paper

It is shown how fluid MHD equations can be used to study the diversion
of the radial current in the accretion disk of a magnetized neutron
star. A self-consistent current system was obtained. When the accretion
flow is in the opposite direction, slight modifications to the previous
analysis can also yield self-consistent current systems.

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