A quasi-static contraction of the inner component in a two-component galaxy model is taken into account form the thermodynamical point of view. An interesting result has achieved at the tidal radius induced by the outer component on the inner one.
Tidal dark matter effect from two-component thermodynamics
SECCO, LUIGI ENRICO
2001
Abstract
A quasi-static contraction of the inner component in a two-component galaxy model is taken into account form the thermodynamical point of view. An interesting result has achieved at the tidal radius induced by the outer component on the inner one.
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