Fig. 9

Temperature derived using the TLS model (TTLS ) using the standard parameters given in Table 4, as a function of temperature derived from a modified black-body fit with a free β parameter (Tfit) in the IRAS 100 μm – Herschel 160, 250, 350, and 500 μm channels (black stars), and in the IRAS 100 μm – Planck 350, 550, and 850 μm channels (gray stars). The triangles show the temperatures derived from a modified black-body fit with β = 2, using the IRAS-Herschel channels (black) and the IRAS-Planck channels (gray). The dashed line corresponds to Tfit = TTLS . The continuous lines show the best polynomial fits.
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