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Peak mass and dynamical friction

A. Del Popolo, M. Gambera

astro-pharXiv:astro-ph/9506067

Abstract

We show how the results given by several authors relatively to the mass of a density peak are changed when small scale substructure induced by dynamical friction are taken into account. The peak mass obtained is compared to the result of Peacock \& Heavens (1990) and to the peak mass when dynamical friction is absent to show how these effects conspire to reduce the mass accreted by the peak.

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