Self-consistent description of axially symmetric magnetospheres of accreting neutron stars

Details Self-consistent description of axially symmetric magnetospheres of accreting neutron stars Self-consistent description of axially symmetric magnetospheres of accreting neutron stars

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..246h&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 246-248 (1984).

Computer Science

Neutron Stars

Scientific paper

We reconsider the problem of spherical accretion onto strongly magnetized compact objects and derive, using ideal MHD, a second order differential equation for the selfconsistent magnetic field structure. Classifying this equation as partly hyperbolic and partly elliptic, we discuss the different region of subsonic, supersonic, superalfvénic and subalfvénic accretion flow.

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