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Oxygen abundances of halo dwarf and subgiant stars from VLT/UVES observations of the [OI] lambda 6300 line
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2001 (English)In: NEW ASTRONOMY REVIEWS, ISSN 1387-6473, Vol. 45, no 8, 545-547 Language: English p.Article in journal (Refereed) Published
Abstract [en]

The forbidden oxygen line at 6300 Angstrom has been observed with UVES on the ESO VLT for 13 dwarf and subgiant stars ranging in metallicity from [Fe/H]similar or equal to -0.7 to - 1.8. The spectra obtained have a resolution of R = 55 000 and SIN similar

Place, publisher, year, edition, pages
ELSEVIER SCI LTD , 2001. Vol. 45, no 8, 545-547 Language: English p.
Keyword [en]
nuclear reactions; nucleosynthesis; abundances; stars; aundances; stars; late-type; galaxy; evolution; METAL-POOR STARS; GIANTS; IRON
Identifiers
URN: urn:nbn:se:uu:diva-37251OAI: oai:DiVA.org:uu-37251DiVA: diva2:65150
Note
Addresses: Nissen PE, Univ Aarhus, Inst Phys & Astron, Aarhus 8000 C, Denmark. Univ Aarhus, Inst Phys & Astron, Aarhus 8000 C, Denmark. European So Observ, D-85748 Garching, Germany. Inst AStron & Space Phys, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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