@inproceedings{discovery10095254, volume = {7}, series = {IAU Symposium Proceedings Series}, year = {2012}, title = {A Multi-wavelength MOCASSIN model of the Magellanic-type galaxy NGC 4449}, number = {284}, editor = {RJ Tuffs and CC Popescu}, month = {January}, booktitle = {Proceedings of the International Astronomical Union}, address = {Preston, UK}, pages = {159--162}, journal = {SPECTRAL ENERGY DISTRIBUTION OF GALAXIES}, note = {This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions.}, publisher = {Cambridge University Press}, abstract = {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 {$\times$} 109L{$\odot$} for the underlying stellar component, Mdust/Mgas of 1/680 and Mdust of 2.2 {$\times$} 106M{$\odot$}.}, author = {Karczewski, OL and Barlow, MJ and Page, MJ and Madden, SC}, url = {https://doi.org/10.1017/S1743921312008976}, issn = {1743-9221}, keywords = {dust, extinction, galaxies: dwarf, galaxies: general, galaxies: individual (NGC 4449), galaxies: stellar content, methods: numerical} }