  Mergers of black holes and other compact objects produce gravitational waves
which carry a part of the energy, momentum, and angular momentum of the system.
Due to asymmetry in the gravitational wave emission, a recoil kick velocity is
imparted to the merger remnant. It has been conjectured that a significant
fraction of the mergers detected so far reside in globular clusters. We explore
the scenario where the merger remnant in a globular cluster is moving at a
significant speed with respect to the binary that underwent merger. We study
this in the situation when the kick velocity is higher than the escape velocity
in the case of globular clusters assuming a Plummer density profile for the
cluster. We study the evolution of the system to study the outcome: whether
dynamical friction can trap the black hole within the globular cluster, whether
the black hole escapes the globular cluster but ends up in the bulge, and
lastly, whether the black halo becomes a halo object. We present results for an
analysis based on orbital parameters of ten globular clusters using data from
GAIA EDR3. We find that if the kick velocity is smaller than $120$ km/s then a
majority of remnant black holes end up in the bulge. Note that our results in
terms of where compact objects launched from a globular cluster end up are
applicable to any mechanism, e.g., a compact object ejected due to three-body
interactions.
