An Observational Hertzsprung–Russell Diagram and Fundamental Parameters of Galactic BA Supergiants
Galactic B- and A-type supergiants serve as critical observational anchors for testing massive-star evolution models and calibrating extragalactic distance indicators. Building upon a uniform Teff scale established in our previous work, we construct a self-consistent observational Hertzsprung–Russell diagram (HRD) for...