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The beryllium abundance in the very metal-poor halo star G 64-12 from VLT/UVES observations
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 364, no 1, L42-L46 p.Article in journal (Refereed) Published
Abstract [en]

We report on a new spectroscopic analysis of the very metal deficient star G 64-12 ([Fe/H] = -3.3), aimed at determining, for the first time, its beryllium content. The spectra were observed during the Science Verification of UVES, the ESO VLT Ultraviolet

Place, publisher, year, edition, pages
SPRINGER-VERLAG , 2000. Vol. 364, no 1, L42-L46 p.
Keyword [en]
stars : Population II; abundances; atmospheres; Galaxy : halo; instrumentation : spectrographs; MODEL ATMOSPHERES; LIGHT-ELEMENTS; ORIGIN; BORON
Identifiers
URN: urn:nbn:se:uu:diva-36657OAI: oai:DiVA.org:uu-36657DiVA: diva2:64556
Note
Addresses: Primas F, European So Observ, Karl Schwarzchild Str 2, D-85748 Garching, Germany. European So Observ, D-85748 Garching, Germany. Uppsala Astron Observ, S-75120 Uppsala, Sweden. Univ Aarhus, Inst Phys & Astron, Aarhus, Denmark.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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