Identifying objects of the optical range in the regions of hard radiation near red dwarf stars
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Abstract
We analyze the localization regions of TeV gamma-ray sources in the X-ray and optical spectral ranges. The angle distances from the position of maxima in the distribution of high-energy fluxes to the probable candidates for identification with red dwarfs are indicated. Possible identifications of fainter TeV sources and other field objects are also considered.
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