Left: fraction of Mdust heated by radiation fields stronger than that of the diffuse ISM (or equivalently by U > Umin) as a function of the L24/LIR ratio for star-formation-dominated sources with EW6.2 > 0.5 μm (black circles) and 0.2 μm <EW6.2 ≤ 0.5 μm (purple circles). The orange line depicts the best fit to the data. Right: dust mass heated by U > Umin versus . Both quantities are normalised by LIR. The purple lines donate the best fit to the data and a scatter of 0.2 dex.
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.