3D hydrodynamics and radiative transfer

Details 3D hydrodynamics and radiative transfer 3D hydrodynamics and radiative transfer

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cemec..45...85b&link_type=abstract

Celestial Mechanics, Volume 45, Issue 1-3, pp. 85-88

Astronomy and Astrophysics

Astrophysics

Scientific paper

Finite difference codes for the solution of the fully three dimensional equations of hydrodynamics, self-gravitation, and radiative transfer have been developed for use on relatively modest computers. Originally developed to study the collapse and fragmentation of protostellar clouds, this family of codes has been used to study a variety of astrophysical problems, with a particular emphasis on cosmogonical issues.

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