What are the internal rotation and mixing properties of intermediateto high-mass stars? KU Leuven
The PhD project covers modelling of large samples of detached eclipsing double-lined spectroscopic or astrometric binaries (EB-SB2) with intermediate- and high-mass components. This will be done for two comparative samples. Both will have an as wide as possible range of orbital periods and will cover masses between 1.3 and 50 solar masses. Sample 1 will contain non-pulsating EB-SB2s while sample 2 will consist of EB-SB2s with non-radial ...