Sun-like stars unlike the Sun: Clues for chemical anomaliesof cool stars

Research output: Research - peer-reviewJournal article

DOI

  • V. Adibekyan
    V. AdibekyanUniversidade do Porto
  • E. Delgado Mena
    E. Delgado MenaUniversidade do Porto
  • S. Feltzing
    S. FeltzingUniversity of Lund, Lund
  • Jonay I. Gonzalez Hernandez
    Jonay I. Gonzalez HernandezUniversidad de La Laguna
  • N. R. Hinkel
    N. R. HinkelVanderbilt University
  • A. J. Korn
    A. J. KornUppsala University Hospital, Uppsala
  • M. Asplund
    M. AsplundRSSS, Australian National University
  • P. G. Beck
    P. G. BeckCEA, CEA, Ctr Saclay, Irfu SPPUniv Paris, Universite Sorbonne Paris Cite-USPC (COMUE), University of Paris Diderot - Paris VII, Lab Interuniv Syst AtmospherUniv Paris 11, Universite Paris Saclay (ComUE), University of Paris Sud - Paris XI, Inst Astrophys SpatialeCNRS Centre National de la Recherche Scientifique
  • Michael Deal
    Michael DealUniversite Federale Toulouse Midi-Pyrenees (ComUE)
  • B. Gustafsson
    B. GustafssonNordita
  • S. Honda
    S. HondaUniv Hyogo
  • K. Lind
    K. LindUppsala Univ, Uppsala University, Dept Phys & AstronUppsala Univ.Uppsala University Hospital, UppsalaMax Planck Inst Astron, Max Planck Society
  • P. E. Nissen
  • L. Spina
    L. SpinaUniversidade de São Paulo
Original languageEnglish
JournalAstronomische Nachrichten
Volume338
Issue number4
Pages (from-to)442-452
Number of pages11
ISSN0004-6337
DOIs
StatePublished - May 2017

    Research areas

  • stars: abundances, stars: chemically peculiar, (stars:) planetary systems, galaxy: abundances, (galaxy:) solar neighborhood, PLANET-HOST STARS, SOLAR TWIN STARS, METAL-POOR STARS, GAIA-ESO SURVEY, HIGH-PRECISION ABUNDANCES, MAIN-SEQUENCE STARS, LTE LINE FORMATION, MILKY-WAY DISK, G-DWARF STARS, T-C TRENDS

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ID: 113973707