The dynamics and cosmogony of galactic coronae

Details The dynamics and cosmogony of galactic coronae The dynamics and cosmogony of galactic coronae

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pazh....1...18a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 1, June 1975, p. 18-22. In Russian.

Astronomy and Astrophysics

Astronomy

2

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

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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