Fig. 8
SED for RN A IRS 1. The triangles show the SOFI JHKs limiting magnitudes as upper limits. The circles show the flux values for IRAC and the WISE 12 and 22 μm fluxes. The best fit is shown with a solid black line, and fits with 
are shown with gray lines. The dashed line is the stellar photosphere of the best fit including the reddening by interstellar extinction.
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