Iron and s-elements abundance variations in NGC 5286: Comparison with 'anomalous' globular clusters and Milky Way satellites

  1. Marino, A.F. 1
  2. Milone, A.P. 1
  3. Karakas, A.I. 1
  4. Casagrande, L. 1
  5. Yong, D. 1
  6. Shingles, L. 1
  7. Da Costa, G. 1
  8. Norris, J.E. 1
  9. Stetson, P.B. 2
  10. Lind, K. 3
  11. Asplund, M. 1
  12. Collet, R. 1
  13. Jerjen, H. 1
  14. Sbordone, L. 45
  15. Aparicio, A. 6
  16. Cassisi, S. 7
  1. 1 Research School of Astronomy and Astrophysics, Australian National University, Mt Stromlo Observatory
  2. 2 Research Canada
    info

    Research Canada

    Ottawa, Canadá

    GRID grid.439950.2

  3. 3 Uppsala University
    info

    Uppsala University

    Upsala, Suecia

    GRID grid.8993.b

  4. 4 Pontificia Universidad Católica de Chile
    info

    Pontificia Universidad Católica de Chile

    Santiago de Chile, Chile

    GRID grid.7870.8

  5. 5 The Milky Way Millennium Nucleus
  6. 6 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    GRID grid.17423.33

  7. 7 Collurania Teramo Observatory
    info

    Collurania Teramo Observatory

    Teramo, Italia

    GRID grid.485976.1

Journal:
Monthly Notices of the Royal Astronomical Society

ISSN: 1365-2966

Year of publication: 2015

Volume: 450

Issue: 1

Pages: 815-845

Type: Article

Export: RIS
DOI: 10.1093/mnras/stv420 SCOPUS: 2-s2.0-84929792053 GOOGLE SCHOLAR lock_openOpen access editor
Data source: Scopus