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The Abundance of Elements in Cool Stars, as Determined from High-Resolution, 1-5 Micron Spectroscopy
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
2005 (English)In: High Resolution Infrared Spectroscopy in Astronomy: eds. H. U. Käufl, R. Siebenmorgen, & A. Moorwood, 365- p.Article, review/survey (Other (popular scientific, debate etc.)) Published
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2005. 365- p.
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URN: urn:nbn:se:uu:diva-77379OAI: oai:DiVA.org:uu-77379DiVA: diva2:105291
Available from: 2006-03-14 Created: 2006-03-14 Last updated: 2011-01-11

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Ryde, NilsGustafsson, BengtEriksson, KjellWahlin, Rurik

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