Open Access

Fig. 7.

image

Cloudy input radiation fields tested. We show the input (dashed) and output (solid) spectral energy distributions for: a continuous star-formation scenario of 10 Myr (with an X-ray component), a Starburst99 instantaneous burst of 3.5 Myr, a Popstar burst of 3.5 Myr, a Magphys fit to the optical-IR photometry. All have model parameters: nH = 102 cm−3, rin = 1020.4 cm, and Zbin = 0.5.

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.