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Dust driven mass loss from carbon stars as a function of stellar parameters. I. A grid of solar-metallicity wind models (Corrigendum)
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
2012 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 546, C1- p.Article in journal (Refereed) Published
Abstract [en]

<BR /> 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. <BR /> Methods: Using exactly the same modelling methods we have recomputed the faulty models with new initial structures. <BR /> 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

Place, publisher, year, edition, pages
edp , 2012. Vol. 546, C1- p.
Keyword [en]
stars: AGB and post-AGB, stars: atmospheres, stars: carbon, circumstellar matter, stars: evolution, errata, addenda
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-196837DOI: 10.1051/0004-6361/200912084eOAI: oai:DiVA.org:uu-196837DiVA: diva2:610957
Available from: 2013-03-13 Created: 2013-03-13 Last updated: 2017-12-06Bibliographically approved

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Wahlin, R.

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