Free Access

Fig. 12


Comparison between model solutions for the dust emission SEDs calculated under the assumption that the emissivity of the young stellar population and the opacity of the associated dust are distributed in a thin disk (solid line) and in a spiral pattern (dashed line), respectively. The solution is for the best fit of NGC 891.

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.