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A primordial star in the heart of the Lion
Caffau E., Bonifacio P., François P., Spite M., Spite F. et al
Astronomy & Astrophysics 542 (2012) A51 - http://hal.archives-ouvertes.fr/hal-00690087
Planète et Univers/Astrophysique/Astrophysique galactique
Physique/Astrophysique/Astrophysique galactique
Planète et Univers/Astrophysique/Astrophysique stellaire et solaire
Physique/Astrophysique/Astrophysique stellaire et solaire
A primordial star in the heart of the Lion
E. Caffau, P. Bonifacio, P. François, M. Spite, F. Spite, S. Zaggia, H. -g. Ludwig, M. Steffen, L. Mashonkina, L. Monaco, L. Sbordone, P. Molaro, R. Cayrel, Bertrand PLEZ ()1, V. Hill, F. Hammer, S. Randich
1 :  LUPM - Laboratoire Univers et Particules de Montpellier
http://web.lupm.univ-montp2.fr/
CNRS : UMR5299 – Université Montpellier II - Sciences et techniques – IN2P3
Université de Montpellier II Place Eugène Bataillon - CC 72 34095 Montpellier Cédex 05
France
Astrophysique Stellaire
Context: The discovery and chemical analysis of extremely metal-poor stars permit a better understanding of the star formation of the first generation of stars and of the Universe emerging from the Big Bang. aims: We report the study of a primordial star situated in the centre of the constellation Leo (SDSS J102915+172027). method: The star, selected from the low resolution-spectrum of the Sloan Digital Sky Survey, was observed at intermediate (with X-Shooter at VLT) and at high spectral resolution (with UVES at VLT). The stellar parameters were derived from the photometry. The standard spectroscopic analysis based on 1D ATLAS models was completed by applying 3D and non-LTE corrections. results: An iron abundance of [Fe/H]=--4.89 makes SDSS J102915+172927 one of the lowest [Fe/H] stars known. However, the absence of measurable C and N enhancements indicates that it has the lowest metallicity, Z<= 7.40x10^{-7} (metal-mass fraction), ever detected. No oxygen measurement was possible. conclusions: The discovery of SDSS J102915+172927 highlights that low-mass star formation occurred at metallicities lower than previously assumed. Even lower metallicity stars may yet be discovered, with a chemical composition closer to the composition of the primordial gas and of the first supernovae.
Anglais
12/03/2012

Astronomy & Astrophysics
internationale
Articles dans des revues avec comité de lecture
08/06/2012
542
A51

LUPM:12-007

Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1203.2607