Nucleosynthesis in AGB stars traced by oxygen isotopic ratios I. Determining the stellar initial mass by means of the 17O/18O ratio ⋆

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1R. de Nutte et al. (>10)
Astronomy & Astrophysics 600, A71 Link to Article [https://doi.org/10.1051/0004-6361/201629195]
1Institute of Astronomy, KU Leuven, Celestijnenlaan 200D B2401, 3001 Leuven, Belgium
e-mail: rutger.denutte@ster.kuleuven.be

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