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The transition from carbon dust to silicate production in low-metallicity asymptotic giant branch and super-asymptotic giant branch stars

✍ Scribed by P. Ventura; M. Di Criscienzo; R. Schneider; R. Carini; R. Valiante; F. D’Antona; S. Gallerani; R. Maiolino; A. Tornambé

No coin nor oath required. For personal study only.

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