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.
1993
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/2499739
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