Fig. 8
10′ × 10′ WISE W1 image of B207 at 3.4 μm. The protostar IRAS 04016+2610 is at the centre of the image. B207 is exhibiting the coreshine effect by showing a clear excess of 3.4 μm emission. The protostar IRAS 04016+2610 is at the centre of the image. B207 is exhibiting the coreshine effect by showing a clear excess of 3.4 μm. The coreshine effect is due to the scattering by large grains inside the globule. The two circular regions marked on the image are the core (C) and rim (R) regions, where we measured optical-, near-, mid-, and far-infrared intensities.
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