EPJ Web Conf.
Volume 208, 2019ISVHECRI 2018 - XX International Symposium on Very High Energy Cosmic Ray Interactions
|Number of page(s)||3|
|Section||Cosmic Ray Experiments (γ-rays)|
|Published online||10 May 2019|
TeV J2032+4130 - very high energy gamma-ray source of unresolved nature
P. N. Lebedev Physical Institute, Russian Academy of Sciences
2 National Research Center “Kurchatov Institute”
* Corresponding author: firstname.lastname@example.org
Published online: 10 May 2019
The Cygnus Region is one of the brightest regions in all ranges of the electromagnetic spectrum and contains a number of potential GeV and TeV emission sources. It includes active star formation regions, pulsars and supernova remnants. Some of the sources have been detected at high and very high energies. One of them discovered due to its proximity to the well-known microquasar Cyg X-3 is the object TeV J2032+4130. This object is still of unresolved nature and is being intensively studied in different energy ranges. The results of twenty-year observations of TeV J2032+4130 by the SHALON experiment are presented in this paper. The collected experimental data on fluxes, spectrum shape and morphology of TeV J2032+413 can help in the future to determine an object type and reveal mechanisms of generation of very high energy emission.
© The Authors, published by EDP Sciences, 2019
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