TY - GEN N2 - 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 6.25 × 109L? for the underlying stellar component, Mdust/Mgas of 1/680 and Mdust of 2.2 × 106M?. SN - 1743-9221 SP - 159 T3 - IAU Symposium Proceedings Series AV - public UR - https://doi.org/10.1017/S1743921312008976 ID - discovery10095254 N1 - This version is the author accepted manuscript. For information on re-use, please refer to the publisher?s terms and conditions. PB - Cambridge University Press KW - dust KW - extinction KW - galaxies: dwarf KW - galaxies: general KW - galaxies: individual (NGC 4449) KW - galaxies: stellar content KW - methods: numerical A1 - Karczewski, OL A1 - Barlow, MJ A1 - Page, MJ A1 - Madden, SC EP - 162 Y1 - 2012/01/01/ CY - Preston, UK TI - A Multi-wavelength MOCASSIN model of the Magellanic-type galaxy NGC 4449 ER -