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Stellar wind properties of O-type stars: mass loss, speeds, structure and quantitative empirical analysis

Boek - Dissertatie

The main focus of this project is to determine the mass loss properties for various populations of hot stars. This will involve using a combination of models developed using the stellar atmosphere+wind code FASTWIND and a range of spectroscopic data. The spectra include young (OB and WNh stars) and older, more evolved cWR stars observed over a range of environments with varying metallicity. This will be the first time this new modelling technique, developed for the MAESTRO project, will be applied to a multi-wavelength, multi-diagnostic study for a statistically significant sample of stars.
Jaar van publicatie:2022