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