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The influence of dust properties on the mass loss in pulsating AGB stars
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2002 (English)In: Radial and Nonradial Pulsations as Probes of Stellar Physics, San Francisco: Astronomical Society of the Pacific , 2002, Vol. 259, 542-545 p.Conference paper, Published paper (Other scientific)
Abstract [en]

We are currently studying carbon based dust types of relevance for carbon-rich AGB stars, to obtain a better understanding of the influence of the optical and chemical properties of the grains on the mass loss of the star. An investigation of the complex

Place, publisher, year, edition, pages
San Francisco: Astronomical Society of the Pacific , 2002. Vol. 259, 542-545 p.
Series
ASP Conference Series
National Category
Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:uu:diva-41629ISBN: 1-58381-099-4 (print)OAI: oai:DiVA.org:uu-41629DiVA: diva2:69530
Available from: 2008-10-17 Created: 2008-10-17

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