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Fig. 7.


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.

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