collaborators

10 papers

astro-ph.GA2026

A Comparative Study of Isothermal Turbulence Statistics: Fourier Space Driving vs. Point Source Driving

Tejahni Desire, Chang-Goo Kim, Rajsekhar Mohapatra

The turbulence driving parameter (; the ratio of the density to velocity fluctuations) is widely used to infer the dominant mode of…

astro-ph.GA2026

Pressure-regulated feedback-modulated star formation as a subgrid model for galaxy formation simulations

Sarah M. R. Jeffreson, Eve C. Ostriker, Chang-Goo Kim +1

We present a new subgrid model for interstellar gas evolution in cosmological simulations of galaxy formation, based on the pressure-regulated, feedback-modulated (PRFM) theory of…

astro-ph.GA2026

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations

Jan D. Burger, Volker Springel, Eve C. Ostriker +7

We introduce PRFM-vol, a new subgrid model for star formation in cosmological simulations that aims to increase the physical realism of cosmological simulations by leveraging resul…

astro-ph.GA2026

Revisiting ram pressure stripping in Wolf-Lundmark-Melotte: No evidence for stripped HI with LGLBS

Daniel R. Rybarczyk, Eric W. Koch, Fabian Caballero Vargas +12

We analyze HI 21-cm observations of the Local Group dwarf galaxy Wolf-Lundmark-Melotte (WLM) from the Local Group L-Band Survey to search for evidence of ram pressure stripping. Wh…

astro-ph.GA2026

Cosmic Ray Feedback in Galactic Disks: Star Formation, Cosmic Ray Transport, and Multiphase Outflows in TIGRESS++ Simulations

Chang-Goo Kim, Lucia Armillotta, Eve C. Ostriker +5

We present new simulations of local star-forming disks that self-consistently evolve cosmic rays (CRs) and multiphase gas using TIGRESS++. To isolate the role of CRs, we conduct pa…

astro-ph.GA2025

Prevention is better than cure? Feedback from high specific energy winds in cosmological simulations with Arkenstone

Jake S. Bennett, Matthew C. Smith, Drummond B. Fielding +6

We deploy the new Arkenstone galactic wind model in cosmological simulations for the first time, allowing us to robustly resolve the evolution and impact of high specific energy wi…