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The analysis of the localization regions of TeV gamma-radiation sources inthe X-ray and optical spectral ranges is carried out. The distances from theposition of the maxima in the distribution of high-energy fluxes to theprobable candidates for identification with red dwarfs are indicated. Possibleidentifications of weaker TeV sources and other field objects are alsoconsidered.

Identification of objects in the optical range in areas of hard radiation near red dwarf stars