Dust production in Circustellar Envelopes (CSEs) of Thermally Pulsing Asymptotic Giant Branch (TP-AGB) Stars
The data here presented are the outputs of the computations
of dust formation in CSEs of TP-AGB stars published in
Nanni et al. 2013 and Nanni et al. 2014. These calculations
are based on the new TP-AGB tracks obtained by the COLIBRI
code (Marigo et al. 2013) in which the characteristic quantities
at the first thermal pulse are taken from the PARSEC
database of full stellar models (Bressan et al. 2012).