| Issue |
A&A
Volume 546, October 2012
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/200912084e | |
| Published online | 01 October 2012 | |
Dust driven mass loss from carbon stars as a function of stellar parameters
I. A grid of solar-metallicity wind models (Corrigendum)
1
Dark Cosmology Centre, Niels Bohr Institute, University of
Copenhagen,
Juliane Maries Vej 30, 2100,
Copenhagen Ø,
Denmark
e-mail: mattsson@dark-cosmology.dk
2
Dept. of Physics and Astronomy, Div. of Astronomy and Space
Physics, Uppsala University, Box
515, 75120
Uppsala,
Sweden
Aims. The purpose of this corrigendum is to point out that a handful of models in the original paper were computed with faulty initial structures.
Methods. Using exactly the same modelling methods we have recomputed the faulty models with new initial structures.
Results. 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
Key words: stars: AGB and post-AGB / stars: atmospheres / stars: carbon / circumstellar matter / stars: evolution / errata, addenda
© ESO, 2012
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