OGLE Collection of Star Clusters. New Objects in the Outskirts of the
  Large Magellanic Cloud
  The Magellanic System (MS), consisting of the Large Magellanic Cloud (LMC),
the Small Magellanic Cloud (SMC) and the Magellanic Bridge (MBR), contains
diverse sample of star clusters. Their spatial distribution, ages and chemical
abundances may provide important information about the history of formation of
the whole System. We use deep photometric maps derived from the images
collected during the fourth phase of The Optical Gravitational Lensing
Experiment (OGLE-IV) to construct the most complete catalog of star clusters in
the Large Magellanic Cloud using the homogeneous photometric data. In this
paper we present the collection of star clusters found in the area of about 225
square degrees in the outer regions of the LMC. Our sample contains 679
visually identified star cluster candidates, 226 of which were not listed in
any of the previously published catalogs. The new clusters are mainly young
small open clusters or clusters similar to associations.
