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The Magellanic System (MS) encompasses the nearest neighbors of the MilkyWay, the Large (LMC) and Small (SMC) Magellanic Clouds, and the MagellanicBridge (MBR). This system contains a diverse sample of star clusters. Theirparameters, such as the spatial distribution, chemical composition and agedistribution yield important information about the formation scenario of thewhole Magellanic System. Using deep photometric maps compiled in the fourthphase of the Optical Gravitational Lensing Experiment (OGLE-IV) we present themost complete catalog of star clusters in the Magellanic System everconstructed from homogeneous, long time-scale photometric data. In this secondpaper of the series, we show the collection of star clusters found in the areaof about 360 square degrees in the MBR and in the outer regions of the SMC. Oursample contains 198 visually identified star cluster candidates, 75 of whichwere not listed in any of the previously published catalogs. The newdiscoveries are mainly young small open clusters or clusters similar toassociations.

OGLE Collection of Star Clusters. New Objects in the Magellanic Bridge and the Outskirts of the Small Magellanic Cloud