Properties of the Hyades, the eclipsing binary HD 27130, and the oscillating red giant ∊ Tauri
Context. The derivation of accurate and precise masses and radii is possible for eclipsing binary stars, allowing for insights into their evolution. When residing in star clusters, they provide measurements of even greater precision, along with additional information on their properties. Asteroseismic investigations of solar-like oscillations
Brogaard, K. et al.
Fecha de publicación:
1
2021