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• W3124405344 abstract "We describe the interplay between stellar evolution and dynamical mass loss of evolving star clusters, based on the principles of stellar evolution and cluster dynamics and on the details of a grid of N-body simulations of Galactic cluster models. The cluster models have different initial masses, different orbits, including elliptical ones, and different initial density profiles. We use two sets of cluster models: one set of Roche lobe filling models and a new set of cluster models that are initially underfilling their tidal radius." @default.
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• W3124405344 date "2010-08-27" @default.
• W3124405344 modified "2023-10-01" @default.
• W3124405344 title "Mass-loss rates and the mass evolution of star clusters" @default.
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• W3124405344 doi "https://doi.org/10.1111/j.1365-2966.2010.17309.x" @default.
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