Fig. B.1

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Estimates of RD = N(DCO+)/N(HCO+) and TK across different studies: estimates in Orion, both single fields and median per bin (green and red circles, respectively; this study), in IRDCs (black diamonds; Miettinen et al. 2011), in high-mass star-forming regions (colour-coded squares; Gerner et al. 2014, 2015, see text for discussion on TK). The black line represents the best fit to the median values of our estimates in Orion and it is exemplified by Eq. B.1.
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