The intermediate neutron capture process - I. Development of the i-process in low-metallicity low-mass AGB stars

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202040170e]

Fig. 10.

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Residual of the best fits for the 14 r/s-stars of Table 2 using our reference 1 M_⊙, [Fe/H] = −2.5 AGB model discussed in this paper that experiences a proton ingestion. The red crosses represent the average values of the residuals. The individual fits are shown in Fig. A.1.

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