API - The Anton Pannekoek Institute for Astronomy
Published May 23, 2022 | Version v1
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The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds

Creators

  • 1. Anton Pannekoek Institute for Astronomy
  • 2. Anton Pannekoek Institute for Astronomy, Institute of Astronomy, KU Leuven
  • 3. Department of Physics and Astronomy University of Sheffield
  • 4. Institute of Astronomy, KU Leuven
  • 5. LMU München
  • 6. Department of Aerospace, Physics and Space Sciences, Florida Institute of Technology
  • 7. Institute of Astronomy, KU Leuven, European Southern Observatory
  • 8. Centro de Astrobiología, CSIC-INTA
  • 9. Argelander-Institut für Astronomie
  • 10. Heidelberger Institut für Theoretische Studien, Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg
  • 11. Armagh Observatory

Description

Supplemental material to 'The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds'. This includes, for each star in the sample: a plot of the observed spectrum overlaid with best fitting models and fitness diagrams for all free parameters. Furthermore we include data (the normalised spectra used in the analysis, and best fitting models) and a basic reproduction package. 

Notes

This publication is part of the project 'Massive stars in low-metallicity environments: the progenitors of massive black holes' with project number OND1362707 of the research TOP-programme, which is (partly) financed by the Dutch Research Council (NWO).

Files

best_models_lineprofiles.zip

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Additional details

Related works

Is part of
Preprint: https://arxiv.org/abs/2202.11080 (URL)
Is supplement to
Journal article: 10.1051/0004-6361/202142742 (DOI)