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The lithium isotope ratio in the metal-poor halo star G271-162 from VLT/UVES observations
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, Vol. 357, no 3, L49-L52 p.Other (Other scientific)
Abstract [en]

A high resolution (lambda/Delta lambda similar or equal to 110 000), very high SIN (greater than or similar to 600) spectrum of the metal-poor turnoff star G 271-162 has been obtained in connection with the commissioning of UVES at VLT/Kueyen. Using both

Place, publisher, year, pages
SPRINGER VERLAG , 2000. Vol. 357, no 3, L49-L52 p.
Keyword [en]
stars : abundances; stars : atmospheres; stars : fundamental parameters; stars : individual : G271-162; ISM : cosmic rays; UVBY-BETA PHOTOMETRY; MODEL ATMOSPHERES; HIGH-VELOCITY; EARLY GALAXY; DISK STARS; HD-84937
Identifiers
URN: urn:nbn:se:uu:diva-36650OAI: oai:DiVA.org:uu-36650DiVA: diva2:64549
Note
Addresses: Nissen PE, Aarhus Univ, Inst Phys & Astron, DK-8000 Aarhus C, Denmark. Aarhus Univ, Inst Phys & Astron, DK-8000 Aarhus C, Denmark. Astron Observ, S-75120 Uppsala, Sweden. European So Observ, D-85748 Garching, Germany.Available from: 2008-10-17 Created: 2008-10-17

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