We present an in depth study on the evolution of galaxy properties in compact groups over the past 3 Gyr .
We are using the largest multi-wavelength sample to-date , comprised 1770 groups ( containing 7417 galaxies ) , in the redshift range of 0.01 < z < 0.23 .
To derive the physical properties of the galaxies we rely on ultraviolet ( UV ) -to-infrared spectral energy distribution modeling , using CIGALE .
Our results suggest that during the 3 Gyr period covered by our sample , the star formation activity of galaxies in our groups has been substantially reduced ( 3-10 times ) .
Moreover , their star formation histories as well as their UV-optical and mid-infrared colors are significantly different from those of field and cluster galaxies , indicating that compact group galaxies spend more time transitioning through the green valley .
The morphological transformation from late-type spirals into early-type galaxies occurs in the mid-infrared transition zone rather than in the UV-optical green valley .
We find evidence of shocks in the emission line ratios and gas velocity dispersions of the late-type galaxies located below the star forming main sequence .
Our results suggest that in addition to gas stripping , turbulence and shocks might play an important role in suppressing the star formation in compact group galaxies .