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In the paper "Excitation Mechanism of Near-Infrared [Fe II] Emission inSeyfert and Starburst Galaxies" by Hideaki Mouri, Kimiaki Kawara, and YoshiakiTaniguchi (ApJ, 528, 186 [2000]), the two panels of Figure 6 were printed intodifferent sizes, as the result of an error in the printing process. The correctversion of Figure 6 appears here.Comment: One postscript file (the correct version of Fig. 6), to appear in Ap

Excitation Mechanism of Near‐Infrared [Feii] Emission in Seyfert and Starburst Galaxies