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• W2146827996 abstract "We present radiative transfer models for submillimeter galaxies with spectroscopic redshifts and mid-infrared spectroscopy from Spitzer/IRS and analyze available Spitzer/MIPS 24, 70 and 160 <i>μ<i/>m data. We use two types of starburst models, a cirrus model and a model for the emission of an AGN torus in order to investigate the nature of these objects. We find that for three of the objects (25%) cirrus emission alone can account for the mid-infrared spectrum and the MIPS and submillimeter data. For the remaining objects we find that we need a combination of starburst and cirrus in order to fit simultaneously the multi-wavelength data. We find that the typical submillimeter galaxy has comparable luminosity in the starburst (median ) and cirrus (median ) components. This could arise if the galaxies have been forming stars continuously for the last 250 Myr with the star formation occurring in the last 5 Myr being shrouded by high-optical-depth molecular cloud dust, whereas the rest of the starlight is attenuated by diffuse dust or cirrus with an <i>A<i/><sub>V<sub/> of about 1 mag." @default.
• W2146827996 created "2016-06-24" @default.
• W2146827996 creator A5045988242 @default.
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• W2146827996 date "2009-06-04" @default.
• W2146827996 modified "2023-10-16" @default.
• W2146827996 title "Starburst and cirrus models for submillimeter galaxies" @default.
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• W2146827996 doi "https://doi.org/10.1051/0004-6361/200811205" @default.
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