153 citations · 433 across the 6 of their papers we have counts for
6 papers
Stellar Populations in STARFORGE: The Origin and Evolution of Star Clusters and Associations
Juan P. Farias, Stella S. R. Offner, Michael Y. Grudić +2
Most stars form in highly clustered environments within molecular clouds, but eventually disperse into the distributed stellar field population. Exactly how the stellar distributio…
What Sets the Star Formation Rate of Molecular Clouds? The Density Distribution as a Fingerprint of Compression and Expansion Rates
Sabrina M. Appel, Blakesley Burkhart, Vadim A. Semenov +3
We use a suite of 3D simulations of star-forming molecular clouds, with and without stellar feedback, magnetic fields, and driven turbulence, to study the compression and expansion…
The dynamics and outcome of star formation with jets, radiation, winds, and supernovae in concert
Michael Y. Grudić, Dávid Guszejnov, Stella S. R. Offner +4
We analyze the first giant molecular cloud (GMC) simulation to follow the formation of individual stars and their feedback from jets, radiation, winds, and supernovae, using the ST…
An Unstable Truth: How Massive Stars get their Mass
Anna L. Rosen, Mark R. Krumholz, Christopher F. McKee +1
The pressure exerted by massive stars' radiation fields is an important mechanism regulating their formation. Detailed simulation of massive star formation therefore requires an ac…
Hybrid Adaptive Ray-Moment Method (HARM): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids
Anna L. Rosen, Mark R. Krumholz, Jeffrey S. Oishi +2
We present a highly-parallel multi-frequency hybrid radiation hydrodynamics algorithm that combines a spatially-adaptive long characteristics method for the radiation field from po…
Gone With the Wind: Where is the Missing Stellar Wind Energy from Massive Star Clusters?
Anna L. Rosen, Laura A. Lopez, Mark R. Krumholz +1
Star clusters larger than contain multiple hot stars that launch fast stellar winds. The integrated kinetic energy carried by these winds is comparable to t…