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Circumstellar H2O in M-type AGB stars
Stockholm University, Faculty of Science, Department of Astronomy.
Stockholm University, Faculty of Science, Department of Astronomy.
2008 (English)In: Organic Matter in Space, 2008, 163-164 p.Conference paper, Published paper (Other academic)
Abstract [en]

Surprisingly high amounts of H2O have recently been reported in the circumstellar envelope around the M-type AGB star W Hya. However, substantial uncertainties remain, as the required radiative transfer modelling is difficult due to high optical depths, sub-thermal excitation and the sensitivity to the combined radiation field from the central star and dust grains.

Place, publisher, year, edition, pages
2008. 163-164 p.
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URN: urn:nbn:se:su:diva-18314DOI: doi:10.1017/S1743921308021455OAI: oai:DiVA.org:su-18314DiVA: diva2:184837
Available from: 2009-01-25 Created: 2009-01-25Bibliographically approved

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Maercker, MatthiasOlofsson, Hans
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