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Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation

By Juan Farias and others at
LogoChalmers University of Technology
and
LogoTata Institute of Fundamental Research
We investigate the dynamical evolution of star clusters during their formation, assuming that they are born from a turbulent starless clump of a given mass that is embedded within a parent self-gravitating molecular cloud characterized by a particular mass surface density. In contrast to the standard practice of most \(N\)-body... Show more
September 12, 2018
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Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation
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