Abstract
AbstractCygnus Region contains many objects that are bright in all wavelengths, including one of the most powerful active star formation regions: Cyg OB2, pulsars, and supernova remnants. Some of the sources have been detected at high and very high energies. One of them was discovered due to the proximity to well‐known microquasar Cyg X‐3. It is an object TeV J2032 + 4130. This object is still of unresolved nature and is being intensively studied in different energy ranges. Numerous X‐ray point sources and diffuse X‐ray emission regions were found within the TeV J2032 + 4130 region by Chandra and Suzaku. Intensities detected in X‐rays from these regions may favor a scenario with the dominantly nucleonic, not electronic origin of TeV emission. The results of the 20‐year observations of TeV J2032 + 4130 object by the SHALON experiment are presented. Collected experimental data on fluxes, spectrum shape, and morphology of TeV J2032 + 413 can help determine an object nature.
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