Stellar Astrophysics Group
The group focuses on understanding astrophysical processes such as magnetic fields, diffusion, convection, and rotation by studying stellar variability, including pulsations and stellar spots. This research is instrumental in comprehending the influence of these processes on the structure and evolution of stars. We utilise data from NASA and ESA missions, including Kepler, TESS, and Gaia, and from ground-based observatories.