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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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    Kelly Lepo (kellylepo@astrodon.social)'s status on Tuesday, 21-Jan-2025 01:35:13 JST Kelly Lepo Kelly Lepo

    And wrapping up my #AAS245 posts - Day 4

    We started off the morning with Stella Offner's plenary Lecture: The Star Formation Engine.

    Offner is part of the STARFORGE collaboration, which simulates the star formation process.

    Star formation involves a lot of physics at a lot of scales — from gravity, magnetic fields, and turbulence that influence how gas collapses into stars, and stellar feedback processes that destroy the surrounding nebula.

    In conversation about 4 months ago from astrodon.social permalink
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