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An analysis of the 2.6 - 3.7 micron spectrum of R Dor
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
2003 (English)In: Mass-losing pulsating stars and their circumstellar matter, 2003Conference paper, Published paper (Other scientific)
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2003.
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URN: urn:nbn:se:uu:diva-71320ISBN: 1-4020-1162-8 (print)OAI: oai:DiVA.org:uu-71320DiVA: diva2:99231
Available from: 2005-05-03 Created: 2005-05-03

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Ryde, Nils

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CiteExportLink to record
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  • apa
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