Fig. B.1
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Comparison of modeled chemical pumping intensities of CH+ using LTE distribution of H2 at the gas temperature and the observed distribution in the Orion Bar. (Top) Modeled intensities for DF3. (Bottom) Modeled intensities for d203-506. Taking into account FUV-pumped levels of H2 is highly important in DF3 compared to d203-506.
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