High-mass eclipsing binaries: A testbed for models of interior structure and evolution
High-mass eclipsing binaries: A testbed for models of interior structure and evolution
Aims. The surface chemical compositions of stars are affected by physical processes that bring the products of thermonuclear burning to the surface. Despite their potential in helping us understand the structure and evolution of stars, elemental abundances are available for only a few high-mass binary stars. We aim to enlarge …