Fig. B.6.
See text for a general description of the figure. NGC 4594: wavelength coverage of HST/STIS spectrum does not include [O I] lines. The [S II] lines have separate narrow profile peaks and a broader profile underneath. A broad component for Hα is to improve the fit. This broad component is also needed for the Palomar spectrum, although a single narrow Gaussian is sufficient for the forbidden lines.
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