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.
H-alpha light maps, velocity maps and velocity profiles for the star-forming gaseous component of random galaxies, from the TNG50 simulation, as in Figure 11 of Pillepich+ (2019). Galaxies with stellar mass above 1010 solar masses are shown at z=1 and z=2. In the three leftmost panels, we show edge-on projections of H-alpha light and mean line-of-sight velocity, in addition to the radial profiles of the mean line-of-sight velocity along the slit depicted by the white solid lines. In the three rightmost panels, we show the face-on projections of H-alpha light and of the line-of-sight velocity dispersion, in addition to the average velocity dispersion profiles along the slit. We always pixelize using square pixels of 0.5 comoving kpc to a side. For each galaxy, two numbers are indicated in the panels: gas rotation velocity (Vrot) and gas dispersion (sigma).
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