Protostars and Planets VI, Heidelberg, July 15-20, 2013

Poster 1S047

An Ensemble of Turbulent Cores

McLeod, Andrew (University of Exeter)
Chabrier, Gilles (École Normale Supérieure de Lyon, CRAL, UMR; University of Exeter)

We present preliminary results from 50 smoothed particle hydrodynamics (SPH) simulations of weakly turbulent cores of molecular gas with turbulent Mach number 0.2, radius 0.13 pc and mass 5 M☉. We use the SEREN code which includes self-gravity and sink particles to model protostars. We use a barotropic equation of state and do not include magnetic fields or radiative transfer due to computational limitations. The cores collapse and fragment, forming protostars; we examine their mass function and binary properties. Each core produces approximately 4 stars with a core mass to star mass efficiency of 25%. The system multiplicity is approximately 40%; cores may produce more than one multiple system.

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