Three-dimensional dynamics of protosellar evolution

Details Three-dimensional dynamics of protosellar evolution Three-dimensional dynamics of protosellar evolution

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phdt.........7c&link_type=abstract

Ph.D. Thesis Los Alamos Scientific Lab., NM.

Astronomy and Astrophysics

Astrophysics

Finite Difference Theory, Protostars, Stellar Evolution, Astrophysics, Cosmology, Rotating Bodies

Scientific paper

A three dimensional finite difference numerical methodology was developed for self-gravitating, rotating gaseous systems. The fully nonlinear equations for time-varying fluid dynamics were solved by a high speed computer in a cylindrical coordinate system rotating with an instantaneous angular velocity, selected such that the net angular momentum relative to the rotating frame was zero. The time dependent adiabatic collapse of gravitationally bound, rotating, protostellar clouds was studied for specified uniform and nonuniform initial conditions.

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