Fig. 9
Left: L′-band image of the surroundings of IRS 10W. The filamentary structure of the NA is appreciated as well as some additional close-by stars with extended emission. Right: the reconstructed SAM image of IRS 10W in L′ band. An asymmetric structure can be seen. Contours represents 10, 20, 30, 40, 50, 60, 70, 80, and 90 % of the peak flux.
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