Understanding the orbital periods of CEMP-s stars | Astronomy & Astrophysics (A&A)

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Fig. 8.

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As Fig. 7 with model sets M6 (dashed line) and M7 (dot-dashed line), in which the angular-momentum loss is computed with Eq. (5) and υ_w = 15 and 7.5 km s⁻¹, respectively, and set M8 (dotted line), in which Eq. (6) is adopted.

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