COSMIC GAMMA-RAY SOURCES AND PROSPECTS OF THEIR OBSERVATIONS WITH INTERNATIONAL COSMIC OBSERVATORY GAMMA-400

被引：0
|
作者：
Beshley, V. [1 ]
Vovk, Ie. [2 ]
Malyshev, D. [3 ]
Marchenko, V. [4 ]
Petruk, O. [1 ]
Savchenko, V. [2 ]
Iakubovskyi, D. [3 ,5 ]
机构：
[1] Inst Appl Problems Mech & Math, 3-b,Naukova St, UA-79060 Lvov, Ukraine
[2] ISDC Data Ctr Astrophys, CH-1290 Chavannes Des Bois, Switzerland
[3] Bogolyubov Inst Theoret Phys, UA-03680 Kiev, Ukraine
[4] Taras Shevchenko Chernigiv Natl Pedag Univ, Astron Sci Res Ctr, UA-14013 Chernigiv, Ukraine
[5] Natl Univ Kyiv Mohyla Acad, UA-04070 Kiev, Ukraine
来源：
JOURNAL OF PHYSICAL STUDIES | 2013年 / 17卷 / 02期
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中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The GAMMA-400 space observatory scheduled to be launched in 2018 by the Russian Space Agency is one of the most interesting forthcoming projects working in the MeV-TeV range. In this paper, we provide a detailed overview of possible scientific opportunities for GAMMA-400, especially concentrating on several topics to which Ukrainian scientific groups can add significant value. These topics include: indirect search of dark matter signatures, determination of parameters of cosmological magnetic fields and studies of a wide class of astrophysical objects such as supernova remnants, active galactic nuclei, gamma-ray bursts and transient gamma-ray sources.
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页数：21
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