Fig. A.5
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Optical depth of the OH lines at 1612, 1665, 1667 and 1720 MHz, as well of H I toward the seven pixels toward G29.935-0.053 of the upGREAT/SOFIA [12C II] observations, as well as accompanying C18O (2–1) (APEX/PI230) and stacked radio recombination lines (40″, GLOSTAR; Brunthaler et al. 2021; Khan et al. 2024). The maps in the middle panel are repeated for clarity from row 2 in Fig. 7.
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