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

TL;DR

This corrigendum revises a set of stellar wind models for carbon stars, correcting initial structures and confirming that the overall trends and conclusions about dust-driven mass loss remain consistent.

Contribution

It provides corrected wind models for carbon stars, ensuring more accurate initial conditions without altering the original study's main conclusions.

Findings

Minor changes in wind property trends

Overall conclusions remain unaffected

Models now based on corrected initial structures

Abstract

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.