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.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)
textMassive stars play a key role in the evolution of the Galaxy; hence they are important objects o...
Context. Stars with masses in excess of 100 M⊙ are observed in the Local Universe, but they remain r...
Spectroscopic analyses of hydrogen-rich WN 5-6 stars within the young star clusters NGC 3603 and R13...
We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of...
Context: The star cluster R136 inside the LMC hosts a rich population of massive stars, including th...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
As most stars are born in a clustered mode, young massive star clusters are the best places to find ...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
The aim of this thesis is to understand the different aspects of the dynamical and stellar evolution...
We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of...
© 2016 The Authors. We introduce a Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograp...
We introduce a Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph (STIS) stellar cens...
International audienceContext. The evolution of massive stars is not fully constrained. Studies of y...
paper accepted in New AstronomyInternational audienceThe evolution of massive stars is only partly u...
textMassive stars play a key role in the evolution of the Galaxy; hence they are important objects o...
Context. Stars with masses in excess of 100 M⊙ are observed in the Local Universe, but they remain r...
Spectroscopic analyses of hydrogen-rich WN 5-6 stars within the young star clusters NGC 3603 and R13...
We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of...
Context: The star cluster R136 inside the LMC hosts a rich population of massive stars, including th...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
As most stars are born in a clustered mode, young massive star clusters are the best places to find ...
Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive ...
The aim of this thesis is to understand the different aspects of the dynamical and stellar evolution...
We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of...
© 2016 The Authors. We introduce a Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograp...
We introduce a Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph (STIS) stellar cens...
International audienceContext. The evolution of massive stars is not fully constrained. Studies of y...
paper accepted in New AstronomyInternational audienceThe evolution of massive stars is only partly u...
textMassive stars play a key role in the evolution of the Galaxy; hence they are important objects o...
Context. Stars with masses in excess of 100 M⊙ are observed in the Local Universe, but they remain r...
Spectroscopic analyses of hydrogen-rich WN 5-6 stars within the young star clusters NGC 3603 and R13...