  We show that gaseous \HI disks of primordial composition irradiated by an
external radiation field can develop a multiphase medium with temperatures
between 10^2 and 10^4 K due to the formation of molecular hydrogen. For a given
\HI column density there is a critical value of the radiation field below which
only the cold \HI phase can exist. Due to a time decreasing quasar background,
the gas starts cooling slowly after recombination until the lowest stable
temperature in the warm phase is reached at a critical redshift $z=z_{cr}$.
Below this redshift the formation of molecular hydrogen promotes a rapid
transition towards the cold \HI phase. We find that disks of protogalaxies with
$10^{20}\simlt N_{HI}\simlt 10^{21} cm^{-2}$ are gravitationally stable at
$T\sim 10^4$ K and can start their star formation history only at $z \simlt
z_{cr}\sim 2$, after the gas in the central portion of the disk has cooled to
temperatures $T\simlt 300$ K. Such a delayed starbust phase in galaxies of low
gas surface density and low dynamical mass can disrupt the disks and cause them
to fade away. These objects could contribute significantly to the faint blue
galaxy population.
