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

关键词：

D O I：

暂无

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.

引用

页数：21

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