The Herschel Dwarf Galaxy Survey - II. Physical conditions, origin of [C II] emission, and porosity of the multiphase low-metallicity ISM

D. Cormier; N. P. Abel; S. Hony; V. Lebouteiller; S. C. Madden; F. L. Polles; F. Galliano; I. De Looze; M. Galametz; A. Lambert-Huyghe

doi:10.1051/0004-6361/201834457

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Volume 626 (June 2019)

A&A, 626 (2019) A23

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Fig. 7.

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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: n_H = 10² cm⁻³, r_in = 10^20.4 cm, and Z_bin = 0.5.

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