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Fig. A.1

image

Average gas density (left) and temperature (right) of the unperturbed disks after 12 Kyr. The solid curves represent the models shown in Fig. 2 (see legend); the dashed curves refer to the corresponding models that include stellar irradiation, as outlined in the text. As expected, beyond some distance from the star, gastemperature is determined by the stellar irradiation temperature.

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