Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
The study of solar-like oscillating red giants in eclipsing binaries (EBs) provides a unique opportunity to advance stellar astrophysics by combining dynamical mass and radius measurements with asteroseismic constraints. EBs provide precise fundamental parameters (e.g. mass, radius, and luminosity) independent of dista...