For low-mass stars, what marks the end of core hydrogen burning and the beginning of the next phase?

Answer

Shell burning ignites in the hydrogen surrounding the helium core

When core hydrogen is exhausted, gravity causes the core to contract, heating the surrounding shell of hydrogen until fusion ignites there, leading to dramatic expansion.

For low-mass stars, what marks the end of core hydrogen burning and the beginning of the next phase?
astrophysicscelestial bodystar evolutionstellar massStar lifecycle