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Tracing AGB Mass Loss by (Synthetic) High-Resolution IR Spectroscopy
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Theoretical Astrophysics.
2007 (English)In: Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes, 2007, 325-326 p.Conference paper, Published paper (Other scientific)
Abstract [en]

We report on recent advances in line profile modelling of different near-infrared (NIR) molecular absorption features based on dynamic model atmospheres for pulsating and mass-losing AGB stars (Mira variables).

Place, publisher, year, edition, pages
2007. 325-326 p.
Identifiers
URN: urn:nbn:se:uu:diva-14296ISBN: 978-1-58381-318-8 (print)OAI: oai:DiVA.org:uu-14296DiVA: diva2:42066
Available from: 2008-01-29 Created: 2008-01-29

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Höfner, Susanne

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