Physical conditions for dust grain alignment in Class 0 protostellar cores - II. The role of the radiation field in models that align and disrupt dust grains

Open Access

Fig. C.1

Effects of the f_high−J parameter on the radiative transfer results at 0.87 mm, with the fixed parameters of a_max = 10 µm and L_★= 20 L_⊙. This corresponds to set II of Table 1. Each column is one radiative transfer run of POLARIS, with f_high−J = 0.0, 0.25, 0.5, 0.75, and 1.0. The top row is the polarized intensity (P), and the bottom row is the polarization fraction.

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