An Optically Thin Inner Accretion Torus around a Weakly Magnetized Neutron Star

Details An Optically Thin Inner Accretion Torus around a Weakly Magnetized Neutron Star An Optically Thin Inner Accretion Torus around a Weakly Magnetized Neutron Star

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pthph..74.1158h&link_type=abstract

Progress of Theoretical Physics, Vol. 74, No. 5, pp. 1158-1160

Physics

Scientific paper

The optically thin inner region around an accreting weakly magnetized
neutron star is examined using the α-model for viscous stress. We
have found that a solution exists only for a limited range of C, an
integration constant in the equation of conservation of angular
momentum.

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