  We consider the Brownian interlacements model in Euclidean space, introduced
by A.S. Sznitman in \cite{sznitman2013scaling}. We give estimates for the
asymptotics of the visibility in the vacant set. We also consider visibility
inside the vacant set of the Brownian excursion process in the unit disc and
show that it undergoes a phase transition regarding visibility to infinity as
in \cite{benjamini2009visibility}. Additionally, we determine the critical
value and that there is no visibility to infinity at the critical intensity.
