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Water Opacity in M Stars
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, 127-128 p.Conference paper (Other scientific)
Abstract [en]

We compare the recently published BT2 water line list tep{2006MNRAS.368.1087B} with other available lists -- NASA Ames tep{partridge:4618} and SCAN tep{2001A&A...372..249J} -- and examine the impact on hydrostatic as well as dynamic models for cool M-type stars. Emerging spectra are compared to ISO-SWS observations of semiregular and Mira variables.

Place, publisher, year, edition, pages
2007. 127-128 p.
URN: urn:nbn:se:uu:diva-14047ISBN: 978-1-58381-318-8OAI: oai:DiVA.org:uu-14047DiVA: diva2:41817
Available from: 2008-01-29 Created: 2008-01-29

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Höfner, Susanne
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Department of Astronomy and Space PhysicsTheoretical Astrophysics

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