The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation, and outflow feedback
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DOI: 10.1093/mnras/stab2338
Abstract: We perform a series of three-dimensional, magnetohydrodynamical simulations of star cluster formation including gravity, turbulence, magnetic fields, stellar radiative heating, and outflow feedback. We observe that the inclusion of protostellar outflows (1) reduces the star… read more here.
Keywords: turbulence magnetic; magnetic fields; turbulence; gravity turbulence ... See more keywords