Massive star asteroseismology with K2 and TESS KU Leuven
Stars born with more than eight times the mass of the Sun contribute significantly to the energetic and chemical evolution of galaxies. Born with convective cores in which they produce new elements through consecutive nuclear fusion cycles, they ultimately collapse leading to potential supernovae and compact objects such as neutron stars and black holes. During the course of their life they are affected by stellar winds, possible binary ...