Fig. 13.
Testing AGN feeding: comparison between star formation activity in the bar and nuclear activity in the host galaxy. Upper panel: SFR in the bar region against bolometric luminosity of the AGN. Lower panel: sSFR in the bar against Eddington ratio. The Spearman’s rank correlation coefficient ρ and its t-value for a null-hypothesis are given in the top left corner of each panel. HE 0045−2145 is not included because it does not host an AGN.
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