Clustered vs. Isolated Star Formation

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I argue that star formation is controlled by supersonic turbulence, drawing for support on a number of 3D hydrodynamical and MHD simulations as well as theoretical arguments. Clustered star formation appears to be a natural result of a lack of turbulent support, while isolated star formation is a signpost of global turbulent support.
7 pages, 5 figures, for publication in ASP Conf. Ser., Modes of Star Formation and the Origin of Field Populations, eds. Grebel & Brandner

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