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

Author: Ventura P.   Di Criscienzo M.   Schneider R.   Carini R.   Valiante R.   D’Antona F.   Gallerani S.   Maiolino R.   Tornambé A.  

Publisher: Oxford University Press

ISSN: 0035-8711

Source: Monthly Notices of the Royal Astronomical Society, Vol.420, Iss.2, 2012-02, pp. : 1442-1456

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content