Mildly suppressed star formation in central regions of MaNGA Seyfert galaxies
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Abstract
Negative feedback from accretion onto super-massive black holes (SMBHs), that
is to remove gas and suppress star formation in galaxies, has been widely
suggested. However, for Seyfert galaxies which harbor less active, moderately
accreting SMBHs in the local universe, the feedback capability of their black
hole activity is elusive. We present spatially-resolved H
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1365-2966
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Science and Technology Facilities Council (ST/M001172/1)