Asteroseismology and Dynamics Reveal Interior Structure and Coeval Evolution in the Triply Post-Main-Sequence system DG Leo

This article reports on research using asteroseismology and dynamics to study the interior structure and evolution of the DG Leo system. The focus is on a triply post-main-sequence system, suggesting a complex and potentially informative dataset for understanding stellar evolution. The use of asteroseismology, which studies stellar oscillations, provides a powerful tool for probing the internal properties of stars.