Star complexes and a scenario for the evolution of spiral galaxiesстатья
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Дата последнего поиска статьи во внешних источниках: 27 мая 2015 г.
Аннотация:
1993AN....314....7C
Abstract
A wide range of the observed properties of disk galaxies can be explained as various dynamical manifestations of collective physical processes in the ensembles of star complexes or gaseous protocomplexes. The proposed cosmological scenario for disk galaxies includes two basic evolutionary stages and their initial conditions; a scenario for spiral formation is developed on these bases.