Neuhäuser, R.; Torres, Guillermo; Mugrauer, M.; Neuhäuser, D. L.; Chapman, J.; Luge, D.; Cosci, M.
(2022)
After core hydrogen burning, massive stars evolve from blue-white dwarfs to red supergiants by expanding, brightening, and cooling within few millennia. We discuss a previously neglected constraint on mass, age, and ...