Free Access

Fig. 9

thumbnail

Differences in the SED resulting from different dust species. The solid line represents the large dust grains and the dashed line the small dust grains. In both cases an unperturbed circumstellar disk of M = 2.67 × 10-2M is used. A G type star hosts this disk with an inner radius of Rin = 38 AU and an outer radius of Rout = 171 AU. In the wavelength range between 730 μm and 3.3 mm, the spectral index for the large grains is αspec,large = 2.84 ± 0.01 and for the small dust grains αspec,small = 3.96 ± 0.01.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.