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Fig. 3


The spectral energy distribution of NGC 4244. The Herschel/SPIRE fluxes from this work (black points) are show together with literature data (red symbols, Dale et al. 2009; MacLachlan et al. 2011). We show the smooth model (blue line); the clumpy model with and without embedded stellar emission (solid and dashed green line, respectively), and the model from MacLachlan et al. (black dotted line).

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