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

Research output: Research - peer-reviewJournal article

DOI

  • A. F. Marino
    A. F. MarinoResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia anna.marino@anu.edu.au
  • A. P. Milone
    A. P. MiloneResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia
  • L. Casagrande
    L. CasagrandeResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia
  • R. Collet
  • A. Dotter
    A. DotterResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia
  • C. I. Johnson
    C. I. JohnsonHarvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA dmilisav@cfa.harvard.edu
  • K. Lind
    K. LindMax-Planck-Institut fuer Astronomie, Koenigstuhl 17, D-69117 Heidelberg, Germany
  • L. R. Bedin
    L. R. BedinINAF-Osservatorio Astronomico di Padova, Vicolo dellOsservatorio 5, I-35122 Padova, Italy
  • H. Jerjen
    H. JerjenResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia
  • A. Aparicio
    A. AparicioInstituto de Astrofísica de Canarias
  • L. Sbordone
    L. SbordoneThe Milky Way Millennium Nucleus, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile
Original languageEnglish
JournalRoyal Astronomical Society. Monthly Notices
Volume459
Issue number1
Pages (from-to)610-623
ISSN0035-8711
DOIs
StatePublished - 1 Jun 2016

    Research areas

  • techniques: photometric, techniques: spectroscopic, stars: Population II, globular clusters: general, globular clusters: individual: NGC104 (47 Tucanae)

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ID: 100185868