Free Access

Fig. 7


Top: A68/HLS115 stellar population SEDs. The Calzetti-based model with nebular emission (green) is plotted together with the SMC-based model (red) for comparison. Although formally the best was obtained with the Calzetti model with no emission, the effects of line emission helped lower the continuum, thus slightly downsizing the physical properties of the population. The curve of the SMC model that produces a much older population illustrates well how much higher the continuum can be without nebular lines. Bottom: A68/HLS115 full and FIR SED fits, in red and green, respectively. The full fit was obtained with an SMG template from M10 with an additional Calzetti-based extinction of AV = 1.2. The FIR fit is obtained with the CE01 library.

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.