Nelson+ (2019) halo-scale gas flow morphologies from TNG50.
Pillepich+ (2019) galaxy kinematic maps from TNG50, stars.
Pillepich+ (2019) galaxy kinematic maps from TNG50, gas.
Rodriguez-Gomez+ (2019) stellar light images and morphological measurements for TNG50.
Rodriguez-Gomez+ (2019) stellar light images for TNG50.
Peroux+ (2020) metallicity vs radial velocity for CGM gas in TNG50.
Pillepich+ (2021) eROSITA-like X-ray bubbles in the CGM of Milky Way/M31-like galaxies in TNG50.
Ramesh+ (2023a) circumgalactic medium of Milky Way/M31-like galaxies in TNG50.
Ramesh+ (2023b) cold clouds in the circumgalactic medium of Milky Way/M31-like galaxies in TNG50.
These figures are similar to Figs 3 and 4 from Rodriguez-Gomez+ (2019), but in this case we extend the analysis (originally for TNG100) to the highly detailed TNG50 simulation. Here we show idealized synthetic images (using Pan-STARRS1 g,r,i filters) of randomly selected galaxies from the TNG50 simulation, generated with the SKIRT radiative transfer code. The text labels indicate the total stellar mass and the 3D stellar half-mass radius.
No more images.