The infrared eye of the wide-field camera 3 on the Hubble Space Telescope reveals multiple main sequences of very low mass stars in NGC2808

  1. Milone, A.P. 12
  2. Marino, A.F. 3
  3. Cassisi, S. 4
  4. Piotto, G. 56
  5. Bedin, L.R. 6
  6. Anderson, J. 7
  7. Allard, F. 8
  8. Aparicio, A. 12
  9. Bellini, A. 7
  10. Buonanno, R. 49
  11. Monelli, M. 12
  12. Pietrinferni, A. 4
  1. 1 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    ROR https://ror.org/03cmntr54

  2. 2 Universidad de La Laguna
    info

    Universidad de La Laguna

    San Cristobal de La Laguna, España

    ROR https://ror.org/01r9z8p25

  3. 3 Max Planck Institute for Astrophysics
    info

    Max Planck Institute for Astrophysics

    Garching bei München, Alemania

    ROR https://ror.org/017qcv467

  4. 4 Collurania Teramo Observatory
    info

    Collurania Teramo Observatory

    Teramo, Italia

    ROR https://ror.org/02ttb5s67

  5. 5 University of Padua
    info

    University of Padua

    Padua, Italia

    ROR https://ror.org/00240q980

  6. 6 Osservatorio Astronomico di Padova
    info

    Osservatorio Astronomico di Padova

    Padua, Italia

    ROR https://ror.org/04z3y3f62

  7. 7 Space Telescope Science Institute
    info

    Space Telescope Science Institute

    Baltimore, Estados Unidos

    ROR https://ror.org/036f5mx38

  8. 8 CRAL, UMR 5574, CNRS, Universit̀e de Lyon, Ècole Normale Supèrieure de Lyon
  9. 9 University of Rome Tor Vergata
    info

    University of Rome Tor Vergata

    Roma, Italia

    ROR https://ror.org/02p77k626

Journal:
Astrophysical Journal Letters

ISSN: 2041-8205

Year of publication: 2012

Volume: 754

Issue: 2

Type: Article

DOI: 10.1088/2041-8205/754/2/L34 SCOPUS: 2-s2.0-84864264073 GOOGLE SCHOLAR lock_openOpen access editor
Data source: Scopus