The C+N+O abundance of ω centauri giant stars: Implications for the chemical-enrichment scenario and the relative ages of different stellar populations

  1. Marino, A.F. 1
  2. Milone, A.P. 23
  3. Piotto, G. 4
  4. Cassisi, S. 5
  5. D'Antona, F. 6
  6. Anderson, J. 7
  7. Aparicio, A. 23
  8. Bedin, L.R. 8
  9. Renzini, A. 8
  10. Villanova, S. 9
  1. 1 Max Planck Institute for Astrophysics
    info

    Max Planck Institute for Astrophysics

    Garching bei München, Alemania

    ROR https://ror.org/017qcv467

  2. 2 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    ROR https://ror.org/03cmntr54

  3. 3 Universidad de La Laguna
    info

    Universidad de La Laguna

    San Cristobal de La Laguna, España

    ROR https://ror.org/01r9z8p25

  4. 4 University of Padua
    info

    University of Padua

    Padua, Italia

    ROR https://ror.org/00240q980

  5. 5 Collurania Teramo Observatory
    info

    Collurania Teramo Observatory

    Teramo, Italia

    ROR https://ror.org/02ttb5s67

  6. 6 Astronomical Observatory of Rome
    info

    Astronomical Observatory of Rome

    Roma, Italia

    ROR https://ror.org/02hnp4676

  7. 7 Space Telescope Science Institute
    info

    Space Telescope Science Institute

    Baltimore, Estados Unidos

    ROR https://ror.org/036f5mx38

  8. 8 Osservatorio Astronomico di Padova
    info

    Osservatorio Astronomico di Padova

    Padua, Italia

    ROR https://ror.org/04z3y3f62

  9. 9 Universidad de Concepción
    info

    Universidad de Concepción

    Concepción, Chile

    ROR https://ror.org/0460jpj73

Journal:
Astrophysical Journal

ISSN: 1538-4357

Year of publication: 2012

Volume: 746

Issue: 1

Type: Article

DOI: 10.1088/0004-637X/746/1/14 SCOPUS: 2-s2.0-84858186787 GOOGLE SCHOLAR lock_openOpen access editor
Data source: Scopus