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Fig. 1


a) High-resolution (18.2′′) column density map of the Taurus B211/B213 region (in units of NH2 cm-2) derived from Herschel data as explained in Appendix A. b) Dust temperature map of the Taurus B211/B213 region (in K) derived at 36.3′′ from Herschel data. Comparison of the two panels shows how dust temperature and column density are anti-correlated.

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