Bibcode
Martínez-Pais, I. G.
Referencia bibliográfica
"Numerical Simulations in Astrophysics, Proceedings of the first UNAM-CRAY Supercomputing
Advertised on:
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1994
Número de citas
0
Número de citas referidas
0
Descripción
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
works. Once the velocity field is determined, a series of line profiles
are numerically computed, under the assumption of a r-α
emissivity law, for different orbital phases and for a range of mass
ratios.