Image Details
Caption: Figure 18.
Same as Figure 16 but for different positions z along the LOS. We consider dust grains with ﹩{S}_{\max }={10}^{6}\,\mathrm{erg}\,{\mathrm{cm}}^{-3}﹩ (left panel) and ﹩{S}_{\max }={10}^{9}\,\mathrm{erg}\,{\mathrm{cm}}^{-3}﹩ (right panel).
© 2022. The Author(s). Published by the American Astronomical Society.