The Herschel Exploitation of Local Galaxy Andromeda (HELGA) - VII. A SKIRT radiative transfer model and insights on dust heating

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Fig. 8

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Dust heating fraction as a function of wavelength for the unevolved stellar populations. The solid black line corresponds to the definition in Eq. (3), the dashed line to Eq. (5). The shaded area between the curves indicates the magnitude of the effect of non-local heating in wavelength space.

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