Physics and modes of star cluster formation

Physics

Scientific paper

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Gravitation, Hydrodynamics, Mhd, Radiative Transfer, Stellar Dynamics, Methods: Numerical, Stars: Formation, Stars: Low-Mass, Brown Dwarfs, Stars: Luminosity Function, Mass Function

Scientific paper

I review the progress made in understanding the physics and modes of
star cluster formation through the use of direct self-gravitating
hydrodynamical simulations, including those that have recently been
performed incorporating radiative transfer and magnetic fields.

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