 An additional "white giant" of type A7 III is the primary of θ² Tauri, a binary system that includes a less massive companion of spectral type A; this pair is visually associated with θ¹ Tauri, one of the four red giants, which also has an A-type binary companion.The remaining population of confirmed cluster members includes numerous bright stars of spectral types A (at least 21), F (about 60), and G (about 50).All these star types are concentrated much more densely within the tidal radius of the Hyades than within an equivalent 10-parsec radius of the Earth.