Showing 1–18 of 18 results
/ Date/ Name
Apr 13, 2021Star Formation Histories from SEDs and CMDs Agree: Evidence for Synchronized Star Formation in Local Volume Dwarf Galaxies over the Past 3 GyrJan 11, 2025FOGGIE X: Characterizing the Small-Scale Structure of the CGM and its Imprint on ObservablesNov 7, 2025Figuring Out Gas & Galaxies In Enzo (FOGGIE). XIV. The Observability of Emission from Accretion and Feedback in the Circumgalactic Medium with Current and Future InstrumentsJun 20, 2022Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^*$ Galaxies is Supported in an Emergent, Non-Hydrostatic EquilibriumFeb 8, 2018Reignition of Star Formation in Dwarf GalaxiesMay 28, 2025Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way AnalogsOct 29, 2025Figuring Out Gas & Galaxies In Enzo (FOGGIE) XI: Circumgalactic O VI Emission Traces Clumpy Inflowing Recycled GasMar 14, 2022Snowmass2021 Cosmic Frontier White Paper: Cosmological Simulations for Dark Matter PhysicsAug 15, 2019The Formation of Ultra-Diffuse Galaxies in the RomulusC Galaxy Cluster SimulationMay 15, 2020The Formation of Isolated Ultra-Diffuse Galaxies in Romulus25Oct 30, 2025Disk Formation and the Size-sSFR Relation of Dwarf GalaxiesOct 31, 2025Figuring Out Gas & Galaxies In Enzo (FOGGIE). XII. The Formation and Evolution of Extended HI Galactic Disks and Warps with a Dynamic CGMOct 31, 2025Figuring Out Gas & Galaxies In Enzo (FOGGIE). XIII. On the Observability of Extended HI Disks and WarpsSep 18, 2023Figuring Out Gas & Galaxies In Enzo (FOGGIE) VII: The (Dis)Assembly of Stellar HalosSep 25, 2024Figuring Out Gas & Galaxies in Enzo (FOGGIE). IX: The Angular Momentum Evolution of Milky Way-like Galaxies and their Circumgalactic GasFeb 20, 2025Are Gas-rich Ultra-diffuse Galaxies and Field Dwarfs Distinct?Jul 28, 2025The Merger-Driven Formation of Classical Low Surface Brightness Galaxies in Romulus25Apr 9, 2024Figuring Out Gas & Galaxies In Enzo (FOGGIE) VIII: Complex and Stochastic Metallicity Gradients at z > 2