116 citations · 998 across the 79 of their papers we have counts for
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Phase mixing due to the Galactic potential: steps in the position and velocity distributions of popped star clusters
G. N. Candlish, R. Smith, M. Fellhauer +3
As star clusters are expected to form with low star formation efficiencies, the gas in the cluster is expelled quickly and early in their development: the star cluster "pops." This…
The Influence of Ram Pressure on the Evolution of Tidal Dwarf Galaxies
R. Smith, P. A. Duc, G. N. Candlish +3
The formation mechanism of tidal dwarf galaxies means they are expected to contain little or no dark matter. As such, they might be expected to be very sensitive to their environme…
Ursa Major II - Reproducing the observed properties through tidal disruption
R. Smith, M. Fellhauer, G. N. Candlish +3
Recent deep photometry of the dwarf spheroidal Ursa Major II's morphology, and spectroscopy of individual stars, have provided a number of new constraints on its properties. With a…