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Negative feedback from accretion onto super-massive black holes (SMBHs), thatis to remove gas and suppress star formation in galaxies, has been widelysuggested. However, for Seyfert galaxies which harbor less active, moderatelyaccreting SMBHs in the local universe, the feedback capability of their blackhole activity is elusive. We present spatially-resolved H$\alpha$ measurementsto trace ongoing star formation in Seyfert galaxies and compare their specificstar formation rate with a sample of star-forming galaxies whose global galaxyproperties are controlled to be the same as the Seyferts. From the comparisonwe find that the star formation rates within central kpc of Seyfert galaxiesare mildly suppressed as compared to the matched normal star forming galaxies.This suggests that the feedback of moderate SMBH accretion could, to someextent, regulate the ongoing star formation in these intermediate to late typegalaxies under secular evolution.

Mildly Suppressed Star Formation in Central Regions of MaNGA Seyfert Galaxies