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Exploiting the data from the GAs Stripping Phenomena in galaxies with MUSE(GASP) program, we compare the integrated Star Formation Rate- Mass relation(SFR-M_ast) relation of 42 cluster galaxies undergoing ram pressure stripping("stripping galaxies") to that of 32 field and cluster undisturbed galaxies.Theoretical predictions have so far led to contradictory conclusions aboutwhether ram pressure can enhance the star formation in the gas disks and tailsor not and until now a statistically significant observed sample of strippinggalaxies was lacking. We find that stripping galaxies occupy the upper envelopeof the control sample SFR-M_ast relation, showing a systematic enhancement ofthe SFR at any given mass. The star formation enhancement occurs in the disk(0.2 dex), and additional star formation takes place in the tails. Our resultssuggest that strong ram pressure stripping events can moderately enhance thestar formation also in the disk prior to gas removal.

Enhanced star formation in both disks and ram pressure stripped tails of GASP jellyfish galaxies