Very high energy gamma-ray emission of TeV J2032+4130 object

被引：0
作者：
Sinitsyna, V. G. [1 ]
Sinitsyna, V. Yu. [1 ]
Balygin, K. A. [1 ,2 ]
Borisov, S. S. [1 ]
Ivanov, I. A. [1 ]
Kirichenko, A. M. [1 ,2 ]
Klimov, A. I. [1 ,2 ]
Kozhukhova, I. P. [1 ]
Mirzafatikhov, R. M. [1 ]
Moseiko, N. I. [1 ,2 ]
Ostashev, I. E. [1 ,2 ]
机构：
[1] Russian Acad Sci, Lebedev Phys Inst, Leninskii Pr 53, Moscow 119991, Russia
[2] Kurchatov Inst, Natl Res Ctr, Pl Akad Kurchatova 1, Moscow 123182, Russia
来源：
BULLETIN OF THE LEBEDEV PHYSICS INSTITUTE | 2017年 / 44卷 / 10期
关键词：
SUPERNOVA-REMNANTS; TELESCOPE; CATALOG; ORIGIN; GALAXY;
D O I：
10.3103/S1068335617100013
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Cygnus Region is known to contain a large number of objects which are bright in all wavelengths including 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 the proximity to well-known microquasar Cyg X-3, is object TeV J2032+4130. This object is still of unresolved nature and is being intensively studied in the different energy ranges. The results of twenty-year observation of TeV J2032+4130 object by the SHALON experiment are presented in this paper. The collected experimental data on fluxes, spectrum shape, and morphology of TeV J2032+4130 can help in the future to determine an object type and to shed light on the source nature.
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页码：277 / 280
页数：4
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