Evolution of thermally pulsing asymptotic giant branch stars - III. Dust production at supersolar metallicities

We extend the formalism presented in our recent calculations of dust ejecta from the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase to the case of super-solar metallicity stars. The TP-AGB evolutionary models are computed with the colibri code. We adopt our preferred scheme for dust growth...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2014-03, Vol.438 (3), p.2328-2340
Hauptverfasser:	Nanni, Ambra, Bressan, Alessandro, Marigo, Paola, Girardi, Léo
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Star & galaxy formation
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