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Fig. B.3.
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Estimates of Tb(74 MHz) – top – and PIMAX(30 GHz) – bottom – of the Orion-Taurus ridge from models of Padovani et al. (2018, 2021). The quantities are derived as a function of ⟨B⊥⟩, a, and E0. The horizontal black dashed lines, with grey errors, represent the corresponding median values reported in Sect. 4.
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