Incompatibility of the continuous steady-state models of pulsar magnetospheres with relativistic magnetohydrodynamics

Details Incompatibility of the continuous steady-state models of pulsar magnetospheres with relativistic magnetohydrodynamics Incompatibility of the continuous steady-state models of pulsar magnetospheres with relativistic magnetohydrodynamics

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.175..645a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 175, June 1976, p. 645-651.

Astronomy and Astrophysics

Astronomy

10

Astronomical Models, Magnetohydrodynamic Flow, Pulsar Magnetospheres, Pulsars, Relativistic Plasmas, Stellar Atmospheres, Conservation Laws, Continuity Equation, Critical Point, Neutron Stars, Steady State

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976MNRAS.175..645A

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