Use Figure 20.5 to find the mass of the white dwarf star that results from the evolution o...

Use Figure 20.5 to find the mass of the white dwarf star that results from the evolution of a 6 M⊙ main sequence star.

FIGURE 20.5 The Masses of the White Dwarf Stars and the Original Masses of the Stars from Which the White Dwarfs Evolve Stars that originally were more massive than about 8 M⊙ can’t produce white dwarfs because their degenerate cores become more massive than the Chandrasekhar limit.