Mass loss and dynamical friction on the Fornax dSph galaxy in the Milky Way potential

Abstract

We study the interplay between mass-loss and dynamical friction (DF) on the orbital decay of the Fornax dwarf spheroidal galaxy in the potential of the Milky Way (MW). Using a simplified single particle approach combined with a mass-loss rate extrapolated by $N-$body simulations we find that the the effect of a time-dependent mass partially compensates DF, and typically produces a much less evident decay of the pergalactic distance, thus confirming that $N-$body simulations in smooth MW potentials without DF can be taken as a good model of the dynamics of dwarf satellite galaxies.

4 pages, 2 figures. To appear in the proceedings of the 398 IAU symposium "MODEST-Compact Stars and Binaries in Dense Star Clusters"