Dynamical zoning within a Lagrangian mesh by use of DYN, a stellar pulsation code

Details Dynamical zoning within a Lagrangian mesh by use of DYN, a stellar pulsation code Dynamical zoning within a Lagrangian mesh by use of DYN, a stellar pulsation code

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977dzwl.book.....c&link_type=abstract

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Physics

Lagrange Coordinates, Pulsars, Stellar Models, Cepheid Variables, Hydrogen Ions, Radiative Transfer

Scientific paper

A method of dynamical zoning within a Lagrangian mesh is used to resolve the motion of the hydrogen ionization front in a time-dependent nonlinear model of a pulsating star. The resulting coupling with the radiative transfer improves the calculated light curves. The method is described in some detail and then applied to a model of the Cepheid eta Aq1.

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