Volume 530, June 2011
|Number of page(s)||5|
|Published online||28 April 2011|
The input disc density structure for model 2 constrained by the fit to the SED (see Tatulli et al. 2011, for details). The gap is filled with a gas at density of nH = 100 cm-3.
|Open with DEXTER|
© ESO, 2011
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