| Issue |
EPJ Web Conf.
Volume 208, 2019
ISVHECRI 2018 - XX International Symposium on Very High Energy Cosmic Ray Interactions
|
|
|---|---|---|
| Article Number | 14009 | |
| Number of page(s) | 3 | |
| Section | Cosmic Ray Experiments (γ-rays) | |
| DOI | https://doi.org/10.1051/epjconf/201920814009 | |
| Published online | 10 May 2019 | |
https://doi.org/10.1051/epjconf/201920814009
TeV J2032+4130 - very high energy gamma-ray source of unresolved nature
1
P. N. Lebedev Physical Institute, Russian Academy of Sciences
2
National Research Center “Kurchatov Institute”
* Corresponding author: sinits@sci.lebedev.ru
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
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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