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Three-Component Modeling of C-Rich AGB Star Winds
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2003 (English)In: Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), 2003, Vol. 15, 53-55 p.Conference paper (Other scientific)
Abstract [en]

The AGB stars are complex systems with interacting radiation, gas and dust processes, all of which an accurate model has to describe properly. Our wind model is based on time-dependent radiation-hydrodynamics combined with a carbon dust component represen

Place, publisher, year, edition, pages
2003. Vol. 15, 53-55 p.
Keyword [en]
hydrodynamics, instabilities, radiative transfer, stars: AGB and post-AGB, stars: mass-loss
URN: urn:nbn:se:uu:diva-44111OAI: oai:DiVA.org:uu-44111DiVA: diva2:72016
Available from: 2008-10-17 Created: 2008-10-17

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