Orbitally-modulated emission line profiles from non-Keplerian accretion disks.
Under the assumption of a vanishingly small pressure and a small viscosity accretion disk in a close binary system, gas streamlines are calculated via an approximate analytical method in the framework of the restricted three body problem. An outer limit for the disk is found, defined by the last non-intersecting orbit, in agreement with previous
Martínez-Pais, I. G.
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1994