  We study the apparition of event horizons in accelerated expanding
cosmologies. We give a graphical and analytical representation of the horizons
using proper distances to coordinate the events. Our analysis is mainly
kinematical. We show that, independently of the dynamical equations, all the
event horizons tend in the future infinity to a given expression depending on
the scale factor that we call asymptotic horizon. We also encounter a subclass
of accelerating models without horizon. When the ingoing null geodesics do not
change concavity in its cosmic evolution we recover the de Sitter and
quintessence-Friedmann-Robertson-Walker models.
