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Star-formation is one of the main processes that shape galaxies, defining itsstellar population and metallicity production and enrichment. It is nowadaysknown that this process is ruled by a set of relations that connect threeparameters: the molecular gas mass, the stellar mass and the star-formationrate itself. These relations are fulfilled at a wide range of scales ingalaxies, from galaxy wide to kpc-scales. At which scales they are broken, andhow universal they are (i.e., if they change at different scales or fordifferent galaxy types) it is still an open question. We explore here how thoserelations compare at different scales using as proxy the new analysis doneusing Integral Field Spectroscopy data and CO observations data from theEDGE-CALIFA survey and the AMUSSING++ compilation.

The local and global relations between $\Sigma_\star$ , $\Sigma_{\rm SFR}$ and $\Sigma_{\rm mol}$ that regulate star-formation