STARFORGE • STAR FORmation in Gaseous Environments • Gizmo, Meshless-Finite-Mass code • Magnetic fields (ideal and non-ideal) • 5-energy bin radiation transfer ("M1") • Dust and gas heating and cooling processes • Star particles with stellar evolution model Stellar feedback: • radiation (heating, pressure, ionization) • stellar winds • protostellar outflows • supernovae • Cosmic-ray transport (single and multi-bin) See Grudic et al. 2021 for methods Senior Personnel Mike Grudic, Pl, Phil Hopkins, Me, Claude-Andre Faucher-Giguere, Anna Rosen Grad Students/Postdocs Shivan Khuller, Nina Filippova, Margot Fitz Axen, Juan Farias, Aleksey Generozov Current or former members of my group @ UT Austin, Nadine Soliman, Piuysh Sharda, Duo Xu, David Guszejnov, PI Now at Ab Initio
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