Fig. 1.
Scheme of the Population III microquasar. When the star fills its Roche lobe, the black hole accretes matter that forms an accretion disk around the compact object. The rate of accretion is very high and the disk becomes thick, expelling an intense wind of particles from the disk. From the innermost region of the disk, powerful relativistic jets are ejected.
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.