Orateur
Dr
Anna Curir
(Astronomical Observatory of Turin - Italy)
Description
We present a set of numerical Nbody simulations to investigate the formation of the outer Milky Way's halo trough accretion events. The aim is to explore the orbital conditions where a retrograde signal in the outer part of the halo can be obtained in order to give a possible explanation of the observed rotational properties of the Milky Way stellar halo.
Author
Dr
Anna Curir
(Astronomical Observatory of Turin - Italy)
Co-auteurs
Dr
Alvaro Villalobos
(Astronomical Observatory of Trieste - Italy)
Mlle
Eva Poglio
(University of Turin -Italy)
Dr
Giuseppe Murante
(Astronomical Observatory of Turin -Italy)
