Numerical simulation of protogalactic eddies

Details Numerical simulation of protogalactic eddies Numerical simulation of protogalactic eddies

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61...18u&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Jan.-Feb. 1984, p. 18-23) Soviet Astronomy (ISSN 0038-5301), vol. 28, Jan.-Feb. 1984, p. 11-

Astronomy and Astrophysics

Astronomy

Astronomical Models, Cosmology, Density Wave Model, Galactic Evolution, Angular Momentum, Computerized Simulation, Galactic Clusters, Galactic Rotation, Gravitational Effects, Nonlinear Equations, Shock Wave Propagation, Spiral Galaxies, Vortices

Scientific paper

Numerical models are developed for protogalactic eddies generated by the passage of large-scale shock fronts during the nonlinear growth phase of gravitational instability in an expanding early universe. The postshock vortex-velocity configurations are determined and the radial distribution of angular momentum K is studied; K will be large enough to account for the rapid rotation of spiral galaxies.

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