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Boron in very metal-poor stars
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
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1998 (English)In: ASTROPHYSICAL JOURNAL, ISSN 0004-637X, Vol. 500, no 1, 241-256 p.Article in journal (Refereed) Published
Abstract [en]

We have observed the B I lambda 2497 line to derive the boron abundances of two very metal-poor stars selected to help in tracing the origin and evolution of this element in the early Galaxy: BD +23 degrees 3130 and HD 84937. The observations were conduct

Place, publisher, year, edition, pages
UNIV CHICAGO PRESS , 1998. Vol. 500, no 1, 241-256 p.
Keyword [en]
Galaxy; evolution; nuclear reactions; nucleosynthesis; abundances; stars; abundances; stars; late-type; stars; Population II; PROPER-MOTION STARS; LI-I LINES; LIGHT-ELEMENTS; PRIMORDIAL NUCLEOSYNTHESIS; HALO STARS; OXYGEN ABUNDANCES; EXTREME SUBDWARFS; EA
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:uu:diva-85309OAI: oai:DiVA.org:uu-85309DiVA: diva2:113217
Addresses: Lopez RJG, Inst Astrofis Canarias, E-38200 La Laguna, Spain. Inst Astrofis Canarias, E-38200 La Laguna, Spain. Univ Texas, Dept Astron, Austin, TX 78712 USA. Uppsala Astron Observ, S-75120 Uppsala, Sweden. Royal Acad Sci, Stockholm Observ, S-13Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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