  The Magellanic System (MS) encompasses the nearest neighbors of the Milky
Way, the Large (LMC) and Small (SMC) Magellanic Clouds, and the Magellanic
Bridge (MBR). This system contains a diverse sample of star clusters. Their
parameters, such as the spatial distribution, chemical composition and age
distribution yield important information about the formation scenario of the
whole Magellanic System. Using deep photometric maps compiled in the fourth
phase of the Optical Gravitational Lensing Experiment (OGLE-IV) we present the
most complete catalog of star clusters in the Magellanic System ever
constructed from homogeneous, long time-scale photometric data. In this second
paper of the series, we show the collection of star clusters found in the area
of about 360 square degrees in the MBR and in the outer regions of the SMC. Our
sample contains 198 visually identified star cluster candidates, 75 of which
were not listed in any of the previously published catalogs. The new
discoveries are mainly young small open clusters or clusters similar to
associations.
