A general, three-dimensional fluid dynamics code for stars in binary systems
We describe the theory and implementation of a three-dimensional fluid dynamics code which we have developed for calculating the surface geometry and circulation currents in the secondaries of interacting binary systems. The main method is based on an Eulerian-Lagrangian scheme to solve the advectiv...
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Format: | Journal article |
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Oxford University Press
2002
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A general three-dimensional fluid dynamics code for stars in binary systems
Published 2002
Journal article