21 citations · 34 across the 4 of their papers we have counts for
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astro-ph.GA2017★ 21 cited
The Role of Stellar Radial Motions in Shaping Galaxy Surface Brightness Profiles
T. Ruiz-Lara, C. G. Few, E. Florido +3
Aims: The physics driving features such as breaks observed in galaxy surface brightness (SB) profiles remains contentious. Here, we assess the importance of stellar radial motions…
astro-ph.GA2017★ 11 cited
The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
B. B. Thompson, C. G. Few, M. Bergemann +39
The typical methodology for comparing simulated galaxies with observational surveys is usually to apply a spatial selection to the simulation to mimic the region of interest covere…