Fig. 2
Mid-infrared diameter of NGC 2264 IRS 1 as a function of wavelength for the 2005 data (crosses) measured with a 90 m baseline and the 2009 data (rectangulars) measured with a 40 m baseline. The values for the diameter in AU (right y-axis) were computed using a distance of 913 pc. Two different models were used: a Gaussian model (black) and a uniform disk model (gray).
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