A systematic study on the properties of aromatic and aliphatic hydrocarbon dust in active galactic nuclei with AKARI near-infrared spectroscopy

Open Access

Fig. 6

(a) Same as Fig. 5a but plotted as a function of L_AGN/L_IR for the AGN sample. (b) Same as Fig. 5a, but L_aromatic/L_IR is replaced with L_aromatic/(L_IR - L_AGN) and plotted for the AGN-dominated galaxies.

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