Fig. 1.
Comparison of the contribution in percentage of the broad component of Hα to the total flux of the Hα − [N II] complex (upper panel) and the FWHM of the very broad component (lower panel) derived in this work vs. C15. Each symbol represents a different LINER as indicated in the legend. The filled (empty) circle represents the two- (three-) component fit to NGC 3245. The gray dashed line is the one-to-one comparison.
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