MAESTRO (Massive Stars Outflows) : The winds of hot massive stars KU Leuven
The winds of hot massive stars through quantitative UV-optical spectroscopy: In this thesis high-quality UV and optical observations collected in the framework of the (XSH)-ULLYSES project will be used to characterize atmospheric and wind properties of massive stars in different metallicity environments. Particular attention will be paid to the surface abundances and the geometrical and dynamical wind properties of these stars using ...