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Broadening of lines of BeII, SrII and BaII by collisions with hydrogen atoms and the solar abundance of strontium
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Astronomy and Space Physics, Observational Astrophysics.
2000 (English)In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, Vol. 311, no 3, p. 535-540Article in journal (Refereed) Published
Place, publisher, year, edition, pages
2000. Vol. 311, no 3, p. 535-540
Keywords [en]
atomic data; line : profiles; Sun : abundances; TRANSITIONS; BERYLLIUM; SPECTRUM; BA+
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URN: urn:nbn:se:uu:diva-36620OAI: oai:DiVA.org:uu-36620DiVA, id: diva2:64519
Available from: 2007-01-09 Created: 2007-01-09 Last updated: 2011-01-14

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Barklem, Paul

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