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Winds of AGB stars: does size matter?
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Astronomy and Space Physics.
2008 (English)In: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. T133, 014007- p.Article in journal (Refereed) Published
Abstract [en]

Asymptotic giant branch (AGB) stars are showing clear signs of significant mass loss through cool stellar winds. These outflows are attributed to the combined effects of pulsation-induced shocks and radiation pressure on dust grains formed in the outer atmospheric layers. This paper gives an overview of the current status of radiation-hydrodynamical modelling of these processes, and presents a toy model that allows analysis of certain features of detailed models, such as the influence of grain size dependent opacities and basic differences in winds of C- and M-type AGB stars.

Place, publisher, year, edition, pages
2008. Vol. T133, 014007- p.
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:uu:diva-149144DOI: 10.1088/0031-8949/2008/T133/014007ISI: 000262583700009OAI: oai:DiVA.org:uu-149144DiVA: diva2:404078
Available from: 2011-03-15 Created: 2011-03-15 Last updated: 2017-12-11Bibliographically approved

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