Free Access

Fig. 11

image

Overview plot of the maximum gap depth in the ideal velocity-channel maps when comparing all transitions considered in this work. The central radiation source is a T Tauri (left) or a Herbig Ae star (right). For the most massive disks in our sample. All considered transitions are optically thick and only trace the surface of the disks. Thus, for the smallest disks the gap is detectable outside the line in the dust continuum (marked with Dust).

This figure is made of several images, please see below:

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.