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Fig. 3.

image

Results of emission line fitting for the inner region of NGC 1672 using a single Gaussian component. From top left to bottom right: flux maps of Brγ λ2.166 μm, [Fe II] λ1.644 μm, H2λ2.12 μm, and He I emission lines. In all of the maps the flux units are 10−20 W m−2. All spatial pixels for which the uncertainty of the emission line fit is higher than 30% are clipped. These pixels are shown in white. North is up and east is to the left.

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