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Fig. 7.

image

Distribution of [hs/ls] as a function of metallicity for the intrinsic S stars of our study (filled squares). The hs-index has been calculated using Ba and Nd, and the ls-index using Y and Zr. The symbols are color-coded with respect to the initial mass in the bins Mini < 1.5 M (blue), 1.5 ≤ Mini < 2.5 M (red), and Mini ≥ 2.5 M (green). We note that these mass bins are designed to match the [hs/ls] STAREVOL predictions only available for Mini = 1.5, 2, 2.5 M. Open circles denote the predictions from pulse to pulse for the different initial masses.

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