Open Access

Fig. 5

image

Download original image

Spectral energy distribution of the circumstellar disk around L1527. Our galario best-fit total flux of the compact Gaussian component for each band, in green, along with longer wavelength VLA measurements from Melis et al. (2011, see Table 4). The protoplanetary disk of L1527 is optically thick up to 3.4 mm (αB7−B3 ~ 2), likely due to its edge-on nature.

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.