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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).
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