Figure 5.
pahfit model fit (black solid line) to the Spitzer IRS spectrum after subtracting field star (filled triangles in cyan) of IRAS 18333−2357, showing several prominent PAH features. The central star continuum, although included in the plot, is too weak to be seen. The blue dashed line represents the dust continuum.

pahfit model fit (black solid line) to the Spitzer IRS spectrum after subtracting field star (filled triangles in cyan) of IRAS 18333−2357, showing several prominent PAH features. The central star continuum, although included in the plot, is too weak to be seen. The blue dashed line represents the dust continuum.

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