1205.6216 (P. Ventura et al.)

Dust formation around AGB and SAGB stars: a trend with metallicity?    [PDF]

P. Ventura, M. Di Criscienzo, R. Schneider, R. Carini, R. Valiante, F. D'Antona, S. Gallerani, R. Maiolino, A. Tornambe

We calculate the dust formed around AGB and SAGB stars of metallicity Z=0.008 by following the evolution of models with masses in the range 1MView original: http://arxiv.org/abs/1205.6216