Searching for Tidal Tails in Galactic Dwarf Spheroidal Galaxies
The formation of the Galactic halo is currently best explained by the combination of two scenarios which previously were regarded as competing models. Based on the kinematics of metal-poor halo field stars, Eggen, Lynden-Bell & Sandage (ELS, 1962) proposed that the halo formed during a rapid, smooth collapse from a homogeneous primordial medium
Martínez-Delgado, David et al.
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