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• W2060168085 abstract "We investigate the dynamical evolution of point-mass systems starting from spheroidal geometry. Such structures may arise as a result of violent compression which results from collisions between clouds of interstellar gas. We use N-body calculations to seek out traces of the initial conditions in their relaxed structures. For initially cold and thick, or thin but hot, systems, the phase of collapse is well described by adiabatic scaling: we show that the axis ratio of stellar clusters grows ∝ R−1/3 during infall, where R is the cluster cylindrical radius. The adiabatic track provides an adequate description of the collapse, provided only that the initial scaleheight of the spheroid, h, is well resolved by the stars: when the mean interparticle distance is larger than h, we find that two-body effects develop rapidly over a single crossing time." @default.
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• W2060168085 date "1999-01-11" @default.
• W2060168085 modified "2023-09-24" @default.
• W2060168085 title "Collapse and evolution of flattened star clusters" @default.
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• W2060168085 doi "https://doi.org/10.1046/j.1365-8711.1999.02153.x" @default.
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