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

Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaperJournal article

DOI

    V. Adibekyan, Universidade do Porto, E. Delgado Mena, Universidade do Porto, S. Feltzing, University of Lund, Lund, Jonay I. Gonzalez Hernandez, Universidad de La Laguna, N. R. Hinkel, Vanderbilt University, A. J. Korn, Uppsala University Hospital, Uppsala, M. Asplund, RSSS, Australian National University, P. G. Beck, CEA, CEA, Ctr Saclay, Irfu SPP, Univ Paris, Universite Sorbonne Paris Cite-USPC (COMUE), University of Paris Diderot - Paris VII, Lab Interuniv Syst Atmospher, Univ Paris 11, Universite Paris Saclay (ComUE), University of Paris Sud - Paris XI, Inst Astrophys Spatiale, CNRS Centre National de la Recherche Scientifique, Michael Deal, Universite Federale Toulouse Midi-Pyrenees (ComUE), B. Gustafsson, Nordita, S. Honda, Univ Hyogo, K. Lind, Uppsala Univ, Uppsala University, Dept Phys & Astron, Uppsala Univ., Uppsala University Hospital, Uppsala, Max Planck Inst Astron, Max Planck Society,
  • P. E. Nissen
  • L. Spina, Universidade 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

See relations at Aarhus University Citationformats

ID: 113973707