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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.

preprint2011arXivOpen access
O. Ł. KarczewskiM. J. BarlowM. J. PageS. C. Madden
astro-ph.CO
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
Citations: 0Reviews: 0Saves: 0Code: not linkedDataset: not linkedInstitutions: 0

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O. Ł. KarczewskiM. J. BarlowM. J. PageS. C. Madden

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