Free Access

Fig. 2


Schematic of the effect of winding up a dipole-like poloidal B field (shown by the vertical arrows) by rotation of the central black hole and accretion disk. The circled dots and circled X’s show the resulting azimuthal B field oriented towards and away from the observer on either side of the jets, and the filled grey arrows show the direction of the associated RM gradients.

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.