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The forbidden abundance of oxygen in the Sun
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2001 (English)In: ASTROPHYSICAL JOURNAL, ISSN 0004-637X, Vol. 556, no 1, L63-L66 p.Article in journal (Refereed) Published
Abstract [en]

We reexamine closely the solar photospheric line at 6300 Angstrom, which is attributed to a forbidden line of neutral oxygen and is widely used in analyses of other late-type stars. We use a three-dimensional time-dependent hydrodynamical model solar atmo

Place, publisher, year, edition, pages
UNIV CHICAGO PRESS , 2001. Vol. 556, no 1, L63-L66 p.
Keyword [en]
Sun : abundances; Sun : photosphere; METAL-POOR STARS; SOLAR-TYPE STARS; B-STARS; CHEMICAL EVOLUTION; LINE FORMATION; ELEMENTS; SPECTRUM; CARBON; GRANULATION; ATMOSPHERES
Identifiers
URN: urn:nbn:se:uu:diva-36655OAI: oai:DiVA.org:uu-36655DiVA: diva2:64554
Note
Addresses: Prieto CA, Univ Texas, McDonald Observ, RLM 15 308, Austin, TX 78712 USA. Univ Texas, McDonald Observ, RLM 15 308, Austin, TX 78712 USA. Univ Texas, Dept Astron, RLM 15 308, Austin, TX 78712 USA. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-13

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