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