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Fig. 4.


Maps of the ratio between the Hα and CO linear normalized flux ratio, line-of-sight velocity difference and velocity dispersion ratio for Centaurus, RXJ1539.5, Abell S1101, Abell 2597, Abell 3581, PKS 0745−191, Abell 1795, RXJ0820.9+0752, 2A0335+096, and Hydra-A from ALMA and MUSE observations. Those maps were made by dividing the corresponding MUSE and ALMA moment maps, respectively. We smoothed the datacube to account for different spatial resolutions (see text for details). Furthermore, the velocity dispersion ratio map shows that, on average, the Hα velocity dispersion is broader than that for CO by a factor of two to three.

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