Free Access
Volume 531, July 2011
Article Number L17
Number of page(s) 5
Section Letters
Published online 05 July 2011

Online material

thumbnail Fig. 3

Model ray tracing images at a wavelength of 350 μm generated with the MCFOST code for combinations of three outer disk sizes and disk inclinations. (top row, from left to right) 200 AU outer disk with inclinations of 0°, 30°, and 60°. (middle row) 300 AU outer disk with same sequence of inclinations. (bottom row) 500 AU outer disk with same sequence of inclinations. Each image has a size of 1200 AU  ×  1200 AU and the pixels match the size of the CSO map pixels. The dynamic range is a factor of 10.

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thumbnail Fig. 4

Simulations of suface density from the N-body numerical model at four wavelengths, increasing from left to right: 24 μm, 70 μm, 350 μm, and 850 μm. The dynamic range is a factor of 10, and the simulation is smoothed to a resolution of 15, matching the capability of ALMA. All figures are contemporaneous in the evolution.

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© ESO, 2011

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