The Pristine survey IV: approaching the Galactic metallicity floor with the discovery of an ultra-metal-poor star

Autor: Piercarlo Bonifacio, D. S. Aguado, A. Arentsen, Eline Tolstoy, Rubén Sánchez-Janssen, Patrick Côté, Elisabetta Caffau, Kim A. Venn, Vanessa Hill, Julio F. Navarro, Nicolas Longeard, Carlos Allende Prieto, Morgan Fouesneau, Pascale Jablonka, Raymond G. Carlberg, Marc Gentile, Federico Sestito, Else Starkenburg, Collin Kielty, Helmer H. Koppelman, Jonay I. González Hernández, Nicolas F. Martin, Kris Youakim, Carmela Lardo, Alan W. McConnachie
Přispěvatelé: Astronomy, Starkenburg E., Aguado D.S., Bonifacio P., Caffau E., Jablonka P., Lardo C., Martin N., Sanchez-Janssen R., Sestito F., Venn K.A., Youakim K., Prieto C.A., Arentsen A., Gentile M., Hernandez J.I.G., Kielty C., Koppelman H.H., Longeard N., Tolstoy E., Carlberg R.G., Cote P., Fouesneau M., Hill V., McConnachie A.W., Navarro J.F., Galaxies, Etoiles, Physique, Instrumentation (GEPI), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Franche-Comté Électronique Mécanique, Thermique et Optique - Sciences et Technologies (UMR 6174) (FEMTO-ST), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS), National Research Council of Canada (NRC), Observatoire astronomique de Strasbourg (ObAS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, 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)
Jazyk: angličtina
Rok vydání: 2018
Předmět:
photometry
stars: abundances
Metallicity
media_common.quotation_subject
1st stars
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
telescope
Star (graph theory)
01 natural sciences
Galactic halo
Metal
hamburg/eso survey
0103 physical sciences
Galaxy formation and evolution
Astrophysics::Solar and Stellar Astrophysics
010306 general physics
010303 astronomy & astrophysics
ComputingMilieux_MISCELLANEOUS
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
media_common
[PHYS]Physics [physics]
Physics
Galaxy: evolution
abundance
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
Astronomy and Astrophysics
stars: abundances
Galaxy: abundances
Galaxy: evolution
Galaxy: formation
Galaxy: halo
Astrophysics - Solar and Stellar Astrophysics
Astrophysics - Astrophysics of Galaxies

model atmospheres
Astrophysics - Astrophysics of Galaxies
chemical-compositions
Universe
sky survey
Galaxy: halo
Galaxy: abundance
Stars
Astrophysics - Solar and Stellar Astrophysics
lithium
13. Climate action
Space and Planetary Science
Galaxy: formation
Astrophysics of Galaxies (astro-ph.GA)
visual_art
visual_art.visual_art_medium
Galaxy: abundances
Astrophysics::Earth and Planetary Astrophysics
halo-stars
Zdroj: Monthly Notices of the Royal Astronomical Society, 481(3), 3838-3852. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 481 (3), pp.3838-3852. ⟨10.1093/mnras/sty2276⟩
ISSN: 1365-2966
0035-8711
DOI: 10.1093/mnras/sty2276
Popis: The early Universe presented a star formation environment that was almost devoid of heavy elements. The lowest metallicity stars thus provide a unique window into the earliest Galactic stages, but are exceedingly rare and difficult to find. Here we present the discovery of an ultra-metal-poor star, Pristine_221.8781+9.7844, using narrow-band Ca H&K photometry from the Pristine survey. Follow-up medium and high-resolution spectroscopy confirms the ultra-metal-poor nature of Pristine_221.8781+9.7844 ([Fe/H] = -4.66 +/- 0.13 in 1D LTE) with an enhancement of 0.3-0.4 dex in alpha-elements relative to Fe, and an unusually low carbon abundance. We derive an upper limit of A(C) = 5.6, well below typical A(C) values for such ultra metal-poor stars. This makes Pristine_221.8781+9.7844 one of the most metal-poor stars; in fact, it is very similar to the most metal-poor star known (SDSS J102915+172927). The existence of a class of ultra metal-poor stars with low(er) carbon abundances suggest that there must have been several formation channels in the early Universe through which long-lived, low-mass stars were formed.
Re-submitted to MNRAS after minor revisions
Databáze: OpenAIRE