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Fig. 4.


Distribution of accretion rate parameter, ℛ = log(Lum[OIII]/MBH, for barred AGN galaxies (dotted line), AGNs in pair systems (dashed line), and unbarred AGNs in the control sample (full surfaces). The solid line represents the ℛ distribution for barred AGN galaxies, using the same parameters, α and β, as for the unbarred galaxies to calculate MBH (see Eq. (2)).

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