Constraints on the H2O formation mechanism in the wind of carbon-rich AGB stars

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Fig. 10

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H₂O abundance profiles for three different chemical models at two different representative abundances at the radius indicated by the dashed vertical line: n_H₂O/n_H₂= 10^-7 in black and n_H₂O/n_H₂= 10^-4 in gray. The Constant abundance profile is a reference model. The Decin/Agúndez profile refers to the results of Decin et al. (2010a) and Agúndez et al. (2010). Cherchneff’s profile refers to her results of 2011. See Sect. 5.2.2 for further details.

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