A Multi-wavelength MOCASSIN Model of the Magellanic-type Galaxy NGC 4449
  We use the photoionisation and dust radiative transfer code MOCASSIN to create a model of the dwarf irregular galaxy NGC 4449. The best-matching model reproduces the global optical emission line fluxes and the observed spectral energy distribution (SED) spanning wavelengths from the UV to sub-mm, and requires the bolometric luminosity of 6.25e9 Lsolar for the underlying stellar component, M_d/M_g of 1/680 and M_d of 2.2e6 Msolar. 
O. {\L}. Karczewski (1), M. J. Barlow (1), M. J. Page (2) and S. C.   Madden (3) ((1) University College London, London, UK,...
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