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

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    A. F. Marino, Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia anna.marino@anu.edu.au, A. P. Milone, Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia, L. Casagrande, Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia,
  • R. Collet
  • A. Dotter, Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia, C. I. Johnson, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA dmilisav@cfa.harvard.edu, K. Lind, Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, D-69117 Heidelberg, Germany, L. R. Bedin, INAF-Osservatorio Astronomico di Padova, Vicolo dellOsservatorio 5, I-35122 Padova, Italy, H. Jerjen, Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia, A. Aparicio, Instituto de Astrofísica de Canarias, L. Sbordone, The 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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