Free Access

Fig. 6


Top: A68/h7 stellar population fits including nebular emission. Here the older Calzetti-based population renders the photometry longwards of 4000 Å well, but fits less the UV, and ultimately the SMC has the smallest . Bottom: full and FIR SED (red and green, respectively). Only M10 templates could produce and in particular = 4.2 for the present SED, attenuated with the SMC law. The peak and width of the dust emission distribution are well fitted here by a R09 template.

This figure is made of several images, please see below:

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.