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Grids of spectra reprocessed by circumstellar dust
The tables of models and spectra reprocessed by dust for carbon-rich stars for the Small and Large Magellanic Clouds (SMC and LMC) computed for two different metallicity values (Z=0.004, Z=0.006) can be downloaded by clicking on the button below.
Two combinations of optical data sets are available, selected as in Nanni et al. 2016 and Nanni 2019.
See Nanni et al. 2019 for a full description of the physical assumptions.
Total dust yields of TP-AGB stellar evolution models as a function of the stellar mass and metallicity (Nanni et al. 2013; Nanni et al. 2014)
Grids of dust yields
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