The GRAVITY young stellar object survey - XV. The star-disk interaction region of the T Tauri star DO Tau

Open Access

Fig. D.3

Corner plot associated with the MCMC process performed on pure-line quantities. The contribution of the halo and the half-width at half maximum for a given velocity v are denoted as $θ_{H W H M}^{v}$ $Mathematical equation: $\theta_{\rm HWHM}^v$$ and C^v_h, and expressed in percentage and mas, respectively.

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.