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Non-standard s-process in massive rotating stars - Yields of 10–150 M⊙ models at Z = 10E−3

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JournalAstronomy & Astrophysics
DateAccepted/In press - 18 Jul 2018
DateE-pub ahead of print (current) - 23 Oct 2018
Early online date23/10/18
Original languageEnglish

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© ESO 2018. This is an author-produced version of the published paper. Uploaded in accordance with the publisher’s self-archiving policy. Further copying may not be permitted; contact the publisher for details.

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