Dust mass abundances obtained fitting the SED of each region using 4 Myr ISRF and Desert dust model. Only fits with a are taken into account. The colour code is the same as in Fig. 5. Dot and dashed lines correspond to the values obtained by Paradis et al. (2011) for typical and bright H ii regions in the LMC modelled assuming a 4 Myr star cluster ISRF and Desert dust model.
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.