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Line formation in solar granulation. VII. CO lines and the solar C and O isotopic abundances
Stockholm University, Faculty of Science, Department of Physics.
Max Planck Institute.
2006 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 456, no 2, 675-688 p.Article in journal (Refereed) Published
Place, publisher, year, edition, pages
2006. Vol. 456, no 2, 675-688 p.
Keyword [en]
convection -- line: profiles -- Sun: abundances -- Sun: photosphere -- Sun: infrared -- solar system: formation
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Astronomy
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URN: urn:nbn:se:su:diva-38218DOI: 10.1051/0004-6361:20064986OAI: oai:DiVA.org:su-38218DiVA: diva2:307835
Available from: 2010-04-01 Created: 2010-04-01 Last updated: 2017-12-12Bibliographically approved

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