Fig. 2.

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Face-on (top row) and edge-on (bottom row) projected properties of the gas component in a CIELO galaxy, as an example. All properties are estimated using the intrinsic properties from the CIELO database and adopting an spaxel scale of s∼1 kpc2. The first column shows the gas-mass weighted distribution. The second column displays the velocity along the LoS for the gas component, whereas the third column illustrates the dispersion of this velocity. The FoV is adjusted to 60×60 kpc2 to encompass the entire galaxy.
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