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Issue A&A
Volume 502, Number 2, August I 2009
Page(s) 541 - 548
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361/200811205
Published online 04 June 2009

A&A 502, 541-548 (2009)
DOI: 10.1051/0004-6361/200811205

Starburst and cirrus models for submillimeter galaxies

A. Efstathiou1 and R. Siebenmorgen2

1  School of Sciences, European University Cyprus, Diogenes Street, Engomi, 1516 Nicosia, Cyprus
    e-mail: a.efstathiou@euc.ac.cy
2  European Southern Observatory, Karl-Schwarzschildstr. 2, 85748 Garching b. München, Germany

Received 21 October 2008 / Accepted 20 May 2009

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 $\mu$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 $L=10^{12.5}~L_\odot$) and cirrus (median $L=10^{12.4}~L_\odot$) 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 $A_{\rm V}$ of about 1 mag.


Key words: galaxies: active -- galaxies: evolution -- galaxies: starburst -- infrared: galaxies



© ESO 2009


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