The Pristine survey XIV: chemical analysis of two ultra-metal-poor stars

Autor: Else Starkenburg, Julio F. Navarro, Lyudmila Mashonkina, Collin Kielty, Piercarlo Bonifacio, K. A. Venn, Pascale Jablonka, A. Arentsen, Nicolas F. Martin, Federico Sestito, Tatyana Sitnova, Carmela Lardo, G. Kordopatis, Elisabetta Caffau, J. I. González Hernández, R. G. Carlberg, David Aguado, Vanessa Hill
Přispěvatelé: Università degli Studi di Bologna, Institute of Astronomy of the Russian Academy of Sciences (INASAN), Russian Academy of Sciences [Moscow] (RAS), EPFL Laboratoire d’astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Instituto de Astrofisica de Canarias (IAC), Universidad de La Laguna [Tenerife - SP] (ULL), University of Victoria [Canada] (UVIC), Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Kapteyn Astronomical Institute [Groningen], University of Groningen [Groningen], Observatoire astronomique de Strasbourg, Université de Strasbourg, CNRS, UMR 7550, 11 rue de l’Université, 67000 Strasbourg, France, Department of Astronomy & Astrophysics [University of Toronto], University of Toronto, Astronomy, Lardo C., Mashonkina L., Jablonka P., Bonifacio P., Caffau E., Aguado D.S., Gonzalez Hernandez J.I., Sestito F., Kielty C.L., Venn K.A., Hill V., Starkenburg E., Martin N.F., Sitnova T., Arentsen A., Carlberg R.G., Navarro J.F., Kordopatis G.
Rok vydání: 2021
Předmět:
stars: abundances
sodium abundance
Analytical chemistry
stellar parameters
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Metal
Galactic halo
hamburg/eso survey
statistical equilibrium
0103 physical sciences
Galaxy formation and evolution
follow-up
Astrophysics::Solar and Stellar Astrophysics
010303 astronomy & astrophysics
milky-way
Astrophysics::Galaxy Astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
Physics
data release
Galaxy: evolution
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
010308 nuclear & particles physics
Astronomy and Astrophysics
model atmospheres
Astrophysics - Astrophysics of Galaxies
Galaxy
equilibrium-line formation
Galaxy: halo
Galaxy: abundance
Radial velocity
Stars
Supernova
Astrophysics - Solar and Stellar Astrophysics
Space and Planetary Science
Galaxy: formation
visual_art
Astrophysics of Galaxies (astro-ph.GA)
visual_art.visual_art_medium
Galaxy: abundances
non-lte
Astrophysics::Earth and Planetary Astrophysics
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 508 (2), pp.3068-3083. ⟨10.1093/mnras/stab2847⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, In press
Monthly Notices of the Royal Astronomical Society, 508(2), 3068-3083. Oxford University Press
ISSN: 0035-8711
1365-2966
DOI: 10.48550/arxiv.2109.14477
Popis: Elemental abundances of the most metal-poor stars reflect the conditions in the early Galaxy and the properties of the first stars. We present a spectroscopic follow-up of two ultra metal-poor stars ([Fe/H]
Comment: 17 pages, 11 figures, accepted for publication in MNRAS
Databáze: OpenAIRE