Dust driven mass loss from carbon stars as a function of stellar parameters - I. A grid of Solar-metallicity wind models (Corrigendum)

The purpose of this corrigendum is to point out that a handful of models in the original paper were computed with faulty initial structures. Using exactly the same modelling methods we have recomputed the faulty models with new initial structures. The new results slightly changes some of the trends in the wind properties with stellar parameters, but the overall effects are small. The conclusions are not affected.

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