What distinguishes the state achieved by the first stage hot core (protostar) immediately after thermal pressure surges?

Answer

It is close to hydrostatic equilibrium, but not yet in thermal equilibrium.

The rising thermal pressure opposes gravity, bringing the object close to hydrostatic equilibrium (pressure balancing gravity), but it is not yet in thermal equilibrium (where fusion balances radiation).

What distinguishes the state achieved by the first stage hot core (protostar) immediately after thermal pressure surges?
gravitystar formationpressurecollapseinterstellar cloud