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Fig. A.8


Pixel to pixel correlation between the G0 value estimated from Tdust, G0(Tdust), using Eqs. ((11)–(13)) map and G0 values estimated from Herschel 70 and 100 μm data, G0(70,100 μm), using Eqs. ((9), (10)) toward a) Aquila; b) Ophiuchus; c) Orion B. The dashed red lines indicate G0(Tdust) = G0(70,100 μm). The solid red lines indicate the best-fit results: G0(Tdust) = (1.38 ± 0.01) × G0(70,100 μm) for Aquila, G0(Tdust) = (0.62 ± 0.01) × G0(70,100 μm) for Ophiuchus, and G0(Tdust) = (2.63 ± 0.09) × G0(70,100 μm) for Orion B. The blue lines in panel c indicate the best-fit result for pixels with G0(Tdust) < 1000: G0(Tdust) = (1.04 ± 0.02) × G0(70,100 μm).

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