Implementation of stellar heating feedback in simulations of star cluster formation: effects on the initial mass function
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DOI: 10.1093/mnras/staa1931
Abstract: Explaining the initial mass function (IMF) of stars is a long-standing problem in astrophysics. The number of complex mechanisms involved in the process of star cluster formation, such as turbulence, magnetic fields and stellar feedback,… read more here.
Keywords: star cluster; cluster formation; feedback; heating ... See more keywords