Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies

It has been suggested that gravitational potential can have a significant role in suppressing star formation in nearby galaxies. To establish observational constraints on this scenario, we investigated the connection between the dynamics - taking the circular velocity curves (CVCs) as a proxy for the inner gravitational potential - and star formation quenching in 215 non-active galaxies across the Hubble sequence from the Calar Alto Legacy Integral Field Area (CALIFA) survey. Our results show that galaxies with similar CVCs tend to have a certain star-formation quenching pattern. To explore these findings in more details, we constructed kiloparsec(kpc)-resolved relations of the equivalent width of the Hα (W<SUB>Hα</SUB>) versus the amplitude (V<SUB>c</SUB>) and shape (β = dlnV<SUB>c</SUB>/dlnR) of the circular velocity at given radii. We find that the W<SUB>Hα</SUB> − V<SUB>c</SUB> is a declining relationship, where the retired regions of the galaxies (the ones with W<SUB>Hα</SUB> values of below 3 Å) tend to have higher V<SUB>c</SUB>. Concurrently, W<SUB>Hα</SUB> − β is a bimodal relationship, which is characterised by two peaks: concentration of the star forming regions at a positive β (rising CVC) and a second concentration of the retired regions with a negative β (declining CVC). Our results show that both the amplitude of the CVC - driven by the mass of the galaxies - and its shape - which reflects the internal structure of the galaxies - play an important role in the quenching history of a galaxy.