Quasi-static evolution of a two component galaxy model is taken into account. The aim is to find a relationship between the tidal radius, induced by the dark matter component on the bright one, and the angular momentum in the two limit cases of late-type and early -type galaxies.
Relationship between tidal radius and angular momentum in a two component disk-galaxy system
SECCO, LUIGI ENRICO
2001
Abstract
Quasi-static evolution of a two component galaxy model is taken into account. The aim is to find a relationship between the tidal radius, induced by the dark matter component on the bright one, and the angular momentum in the two limit cases of late-type and early -type galaxies.File in questo prodotto:
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