Radial velocity A) and the ratio of the radial velocity to the escape velocity B) of sink particles for different values of β0 are plotted as a function of radius, at the epoch when the stellar system has accreted ≈30 M⊙. Some protostars with higher β0 move away from the cluster, with the radial velocity exceeding the escape velocity.
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.