Volume 546, October 2012
|Number of page(s)||1|
|Section||Interstellar and circumstellar matter|
|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)
Dark Cosmology Centre, Niels Bohr Institute, University of
Juliane Maries Vej 30, 2100,
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.