Galaxies are idealized as gas/star homogeneous spheroids in quasi static contraction within embedding dark matter homogeneous spheroids, aiming to see to what extent the dynamical properties and the final morphology of the baryonic subsystem are affected by tidal interactions induced by the non baryonic subsystem.
Tidal Effects of a Massive Spheroidal Halo on an Inner Spheroidal Contracting Visible Body - Application to an Evolutionary Disk / Galaxy Model
CAIMMI, ROBERTO;SECCO, LUIGI ENRICO
1993
Abstract
Galaxies are idealized as gas/star homogeneous spheroids in quasi static contraction within embedding dark matter homogeneous spheroids, aiming to see to what extent the dynamical properties and the final morphology of the baryonic subsystem are affected by tidal interactions induced by the non baryonic subsystem.File in questo prodotto:
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