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Fig. 6


HD 100546 disk physical structure from Kama et al. (2016). Top left and moving clockwise: dust temperature (K), gas temperature (K), UV flux (in units of the interstellar radiation field) and number density (cm−3 ). The two white contours in each of the temperature plots correspond to a temperature of 30 and 50 K. The shaded region highlights the location of the SO motivated by RADEX calculations and used in the LIME modelling.

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