In very massive stars (at least eight times the Sun's mass), what sequence of fusion follows helium burning in the core?

Answer

Carbon, then neon, oxygen, and silicon fusion in successive shells

In stars much more massive than the Sun, after helium is exhausted, the core contracts and ignites successive burning stages: carbon, then neon, oxygen, and silicon, forming onion-like shells.

In very massive stars (at least eight times the Sun's mass), what sequence of fusion follows helium burning in the core?
ElementastronomystarFusionnucleosynthesis