153 citations · 1.3k across the 37 of their papers we have counts for
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Less wrong: a more realistic initial condition for simulations of turbulent molecular clouds
Henry B. Lane, Michael Y. Grudić, Dávid Guszejnov +3
Simulations of isolated giant molecular clouds (GMCs) are an important tool for studying the dynamics of star formation, but their turbulent initial conditions (ICs) are uncertain.…
The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds
Sabrina M. Appel, Blakesley Burkhart, Vadim A. Semenov +2
Using a suite of 3D hydrodynamical simulations of star-forming molecular clouds, we investigate how the density probability distribution function (PDF) changes when including gravi…
Blowing Bubbles around Intermediate-Mass Stars: Feedback from Main-Sequence Winds is not Enough
Anna L. Rosen, Stella S. R. Offner, Michael M. Foley +1
Numerous spherical ``shells" have been observed in young star-forming environments that host low- and intermediate-mass stars. These observations suggest that these shells may be p…
Dust in the Wind with Resonant Drag Instabilities: I. The Dynamics of Dust-Driven Outflows in GMCs and HII Regions
Philip F. Hopkins, Anna L. Rosen, Jonathan Squire +4
Radiation-dust driven outflows, where radiation pressure on dust grains accelerates gas, occur in many astrophysical environments. Almost all previous numerical studies of these sy…