Fig. 8
Mass of a distinctly chosen gas knot in the wake of ram-pressure stripped galaxy 1nb in simulation #7 is shown with respect to simulation time. The gas clump is formed after 160 Myr of the onset of the ram pressure. Until the end of the simulation, the gas knot loses half of its mass due to star formation as shown in a). The mass of newly formed stars, present in the gas knot, is displayed in b).
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.