The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds

The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds

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...

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Bibliographische Detailangaben
Hauptverfasser: Brands, Sarah A., de Koter, Alex, Bestenlehner, Joachim M., Crowther, Paul A., Sundqvist, Jon O., Puls, Joachim, Caballero-Nieves, Saida M., Abdul-Masih, Michael, Driessen, Florian a., García, Mariam, Geen, Sam, Graefener, Goetz, Hawcroft, Calum, Kaper, Lex, Keszthelyi, Zsolt, Langer, Norbert, Sana, Hugues, Schneider, Fabian R. N., Shenar, Tomer, Vink, Jorick S.
Format: Dataset
Sprache:eng
Schlagworte:
massive stars, stellar winds, clumping, mass-loss, Magellanic Cloud Cloud, R136
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Zusammenfassung: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.
DOI:10.5281/zenodo.6353512