The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136

  1. Bestenlehner, J.M. 1
  2. Crowther, P.A. 1
  3. Caballero-Nieves, S.M. 12
  4. Schneider, F.R.N. 34
  5. Simón-Díaz, S. 56
  6. Brands, S.A. 7
  7. De Koter, A. 78
  8. Gräfener, G. 9
  9. Herrero, A. 56
  10. Langer, N. 9
  11. Lennon, D.J. 56
  12. Maíz Apellániz, J. 10
  13. Puls, J. 11
  14. Vink, J.S. 12
  1. 1 University of Sheffield
    info

    University of Sheffield

    Sheffield, Reino Unido

    GRID grid.11835.3e

  2. 2 Department of Aerospace, Physics and Space Sciences, Florida Institute of Technology
  3. 3 Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg
  4. 4 Heidelberger Institut für Theoretische Studien
  5. 5 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    GRID grid.17423.33

  6. 6 Universidad de La Laguna
    info

    Universidad de La Laguna

    San Cristobal de La Laguna, España

    GRID grid.10041.34

  7. 7 University of Amsterdam
    info

    University of Amsterdam

    Ámsterdam, Holanda

    GRID grid.7177.6

  8. 8 University of Leuven
    info

    University of Leuven

    Lovaina, Bélgica

    GRID grid.5596.f

  9. 9 University of Bonn
    info

    University of Bonn

    Bonn, Alemania

    GRID grid.10388.32

  10. 10 Centro de Astrobiología
    info

    Centro de Astrobiología

    Madrid, España

    GRID grid.462011.0

  11. 11 Ludwig Maximilian University of Munich
    info

    Ludwig Maximilian University of Munich

    Múnich, Alemania

    GRID grid.5252.0

  12. 12 Armagh Observatory and Planetarium
Journal:
Monthly Notices of the Royal Astronomical Society

ISSN: 1365-2966

Year of publication: 2020

Volume: 499

Issue: 2

Pages: 1918-1936

Type: Article

Export: RIS
DOI: 10.1093/mnras/staa2801 SCOPUS: 2-s2.0-85096748875 GOOGLE SCHOLAR
Data source: Scopus