Fig. 5

Download original image
Morphological structure of an interstellar ice. Top panels: accretion rate during the molecular cloud collapse. Bottom panels: fractional ice composition AN as a function of the ice thickness (in ML). Left-hand side column: fast flow. Right-hand side column: slow flow. Black indicates H2O, orange represents NH3, and blue symbolizes CO. Red lines are for the cloud thermal profile. Dashed lines in the bottom panels represent the case in which gas and dust temperatures differ (Tg – Td = 50 K).
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.