Asymptotic giant branch stars in the Large Magellanic Cloud: evolution of dust in circumstellar envelopes
We calculated theoretical evolutionary sequences of asymptotic giant branch (AGB) stars, including the formation and evolution of dust grains in their circumstellar envelopes. By considering stellar populations of the Large Magellanic Cloud (LMC), we calculate synthetic colour-colour and colour-magnitude diagrams, which are compared with those
Dell'Agli, F. et al.
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2015