Three-Component Modeling of C-Rich AGB Star Winds
2003 (English)In: Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), 2003, Vol. 15, 53-55 p.Conference paper (Other scientific)
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.
hydrodynamics, instabilities, radiative transfer, stars: AGB and post-AGB, stars: mass-loss
IdentifiersURN: urn:nbn:se:uu:diva-44111OAI: oai:DiVA.org:uu-44111DiVA: diva2:72016