Fig. 9
Submillimeter brightness profiles of AFGL 2591 measured with JCMT/SCUBA (error bars), and synthetic brightness profiles derived from WR models and convolved by the SCUBA beams for p = 1.0 (solid line) and p = 1.5 (dashed line). The vertical dotted line indicates the adopted source radius. For this source, we choose a density profile of p = 1.0.
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