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  -