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Fig. 6

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Spectra of the LINERs with a clear BLR, in addition to NGC 4203 presented above, modeled using [O I] as template for the narrow lines. The broad Hα (red curve) is reproduced with a skewed Gaussian. The original spectrum is in black, the individual narrow lines are in blue, the total line emission in green, the residuals in red. Wavelengths are in Å, while fluxes are in units of 10-18erg s-1 cm-2 Å-1.

This figure is made of several images, please see below:

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