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The studies of FUors, EXors, and other young eruptive stars are very important for understanding the earliest stages of pre-main-sequence evolution. We describe the current situation in this field. This is a short version of thereview presented at the conference "Non-Stationary Processes in the Protoplanetary Disks and Their Observational Manifestations" held at the Crimean Astrophysical Observatory.doi:10.34898/aat.vol3.iss3.pp4-7 fatcat:n7jva2mg3jdjrk73ofplzvl6se