185 citations · 545 across the 9 of their papers we have counts for
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What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations
Mark R. Krumholz, Andrew T. Myers, Richard I. Klein +1
As star-forming clouds collapse, the gas within them fragments to ever-smaller masses. Naively one might expect this process to continue down to the smallest mass that is able to r…
The CH+ Abundance in Turbulent, Diffuse Molecular Clouds
Andrew Myers, Christopher McKee, Pak Shing Li
The intermittent dissipation of interstellar turbulence is an important energy source in the diffuse ISM. Though on average smaller than the heating rates due to cosmic rays and th…
Star Cluster Formation in Turbulent, Magnetized Dense Clumps with Radiative and Outflow Feedback
Andrew Myers, Richard Klein, Mark Krumholz +1
We present three Orion simulations of star cluster formation in a 1000 Msun, turbulent molecular cloud clump, including the effects of radiative transfer, protostellar outflows, an…