Dynamics and cosmogony of galaxy halos

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Coronas, Galactic Evolution, Galactic Structure, Contraction, Density Distribution, Dynamic Models, Energy Dissipation, Gravitational Effects, Hydrogen Clouds

Scientific paper

A simple stellar-dynamic model of galactic coronae is considered which
has nearly radial motions and an inverse-square density law. Processes
are examined by which these systems became spherical and underwent
quasi-steady contraction at the early evolutionary stage when they were
still basically gaseous.

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