Scaling relations investigated here as a function of environment and process. From left to right: SFR-mass, size-mass, H2-mass, and HI-mass. Only isolated galaxies with no process are considered and the best fit of the relation is shown. This line is used as reference in the following analysis. In the SFR-mass plot, the separation used to identify star forming and passive galaxies (log(SSFR[yr⁻¹]) = −11) is also shown.