Chemical abundances in the multiple sub-giant branch of 47 Tucanae: Insights on its faint sub-giant branch component

  1. Marino, A.F. 1
  2. Milone, A.P. 1
  3. Casagrande, L. 1
  4. Collet, R. 12
  5. Dotter, A. 1
  6. Johnson, C.I. 3
  7. Lind, K. 4
  8. Bedin, L.R. 5
  9. Jerjen, H. 1
  10. Aparicio, A. 6
  11. Sbordone, L. 78
  1. 1 Australian National University
    info

    Australian National University

    Canberra, Australia

    GRID grid.1001.0

  2. 2 Aarhus University
    info

    Aarhus University

    Århus, Dinamarca

    GRID grid.7048.b

  3. 3 Harvard-Smithsonian Center for Astrophysics
    info

    Harvard-Smithsonian Center for Astrophysics

    Cambridge, Estados Unidos

    GRID grid.455754.2

  4. 4 Max Planck Institute for Astronomy
    info

    Max Planck Institute for Astronomy

    Heidelberg, Alemania

    GRID grid.429508.2

  5. 5 Osservatorio Astronomico di Padova
    info

    Osservatorio Astronomico di Padova

    Padua, Italia

    GRID grid.436939.2

  6. 6 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    GRID grid.17423.33

  7. 7 Pontificia Universidad Católica de Chile
    info

    Pontificia Universidad Católica de Chile

    Santiago de Chile, Chile

    GRID grid.7870.8

  8. 8 The Milky Way Millennium Nucleus
Journal:
Monthly Notices of the Royal Astronomical Society

ISSN: 1365-2966

Year of publication: 2016

Volume: 459

Issue: 1

Pages: 610-623

Type: Article

Export: RIS
DOI: 10.1093/mnras/stw611 SCOPUS: 2-s2.0-84969769810 GOOGLE SCHOLAR lock_openOpen access editor
Data source: Scopus