Showing 21–40 of 96 results
/ Date/ Name
Feb 3, 2023Orbital Evolution of Binaries in Circumbinary DisksJun 6, 2019The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNGApr 15, 2019High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functionsDec 18, 2018The star-formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematicsSep 19, 2020DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or StretchedJan 28, 2021Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST ObservationsJan 28, 2021The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversityDec 3, 2020How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relicsNov 14, 2017The evolution of the mass-metallicity relation in IllustrisTNGAug 10, 2023Star Formation Shut Down by Multiphase Gas Outflow in a Galaxy at a Redshift of 2.45Jun 5, 2025Probing neutral outflows in z ~ 2 galaxies using JWST observations of Ca II H and K absorption linesMay 27, 2019A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observationsSep 30, 2019Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG SimulationsMay 19, 2020Resolving small-scale cold circumgalactic gas in TNG50Dec 13, 2018The IllustrisTNG Simulations: Public Data ReleaseMay 23, 2022Sunyaev-Zel'dovich effect and X-ray scaling relations of galaxies, groups and clusters in the IllustrisTNG simulationsDec 17, 2018The Sunyaev-Zel'dovich effect of simulated jet-inflated bubbles in clustersFeb 14, 2019First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedbackMar 26, 2019Imprint of Drivers of Galaxy Formation in the Circumgalactic MediumJan 17, 2023Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations