Fig. 3
Face-on images of gas surface density of an isolated disk galaxy simulation using gasoline (left) and ramses (right). The characteristic sizes of gas structures are larger in ramses than in gasoline due partly to the Jeans polytrope pressure floor implemented in ramses and partly to differences in more fundamental aspects of the codes (e.g., hydrodynamic or gravity solvers).
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.