Four barred AGN galaxies show C(Hα)/C(CO) ratios of 0.3-0.4 while 13 others show ratios near 1, interpreted as AGN feedback suppressing central star formation after bar-driven gas accumulation.
The lat- ter two are sub-classes of quenching galaxies
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Suppression of star formation at the centre of barred AGN galaxies
Four barred AGN galaxies show C(Hα)/C(CO) ratios of 0.3-0.4 while 13 others show ratios near 1, interpreted as AGN feedback suppressing central star formation after bar-driven gas accumulation.