Free Access

Fig. 8


Artistic rendition depicting the IR H-band emission determined for γ Cas. We show the derived extent, elongation, and position angle of the Gaussian disk. The inner region is optically thick. Neither partial obscuration of the star by the disk nor the star’s gravity-darkening are included in the MIRC model.

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.