Dynamics of Star Clusters and the Milky Way

By S. Deiters, B. Fuchs, Andreas Just, Rainer Spurzem, R. Wielen. 2001

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The Runaway Growth of Intermediate-Mass Black Holes in Dense Star Clusters (2002, methodology): “RESULTS OF N-BODY SIMULATIONS The development of the GRAPE family of special-purpose computers makes it relatively straightforward to test and tune the above simple model using directN-body calculations.”
Direct N-body Modelling of Stellar Populations: Blue Stragglers in M67 (2000, methodology): “Our approach in this area is to include a consistent treatment of stellar and binary evolution in a state-of-the-art N-body code so as to allow the generation and interaction of the full range of stellar populations within a cluster environment (Hurley et al. 2000).”
Observations of Thick Disks in the Hubble Space Telescope Ultra Deep Field (2006, background): “Subject headinggs: galaxies: formation — galaxies: high-redshift — galaxies: spiral Online material: color figures”
HCN and HCO+ Observations of the Galactic Circumnuclear Disk (2005, background): “Several stellar populations are observed within the central parsec (Genzel 2001).”
Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue (2009, background): “A major study of the Hyades cluster as based on the first Hipparcos catalogue was presented by Perryman et al. (1998), and further studies based on the same data by Madsen et al. (2000), Madsen et al. (2001) and de Bruijne et al. (2001).”