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An Approximate Solver for Riemann and Riemann-like Ellipsoidal Configurations

© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Shangli Ou 2006 ApJ 639 549 DOI 10.1086/499268

0004-637X/639/1/549

Abstract

We introduce a new technique for constructing three-dimensional models of incompressible Riemann S-type ellipsoids and compressible triaxial configurations that share the same velocity field as that of Riemann S-type ellipsoids. Our incompressible models are exact steady-state configurations; our compressible models represent approximate steady-state equilibrium configurations. Models built from this method can be used to study a variety of relevant astrophysical and geophysical problems.

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10.1086/499268