TEV EMISSION FROM CLOSE BINARIES

被引：13

作者：

MOSKALENKO, IV

机构：

[1] International Centre for Theoretical Physics, Trieste

来源：

SPACE SCIENCE REVIEWS | 1995年 / 72卷 / 3-4期

关键词：

D O I：

10.1007/BF00749007

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It is commonly accepted that candidates for very high energy gamma-ray sources are neutron stars, binary systems, black holes etc. Close binary systems containing a normal hot star and a neutron star (or a black hole) form an important class of very high energy gamma-ray sources. Such systems are variable in any region of the electromagnetic spectrum and they enable us to study various stages of stellar evolution, accretion processes, mechanisms of particle acceleration, etc. Phenomena connected with this class of very high energy gamma-ray sources are discussed. Particular emphasis has been placed on the TeV energy region.

引用

页码：593 / 627

页数：35

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[61] PARAMETERS OF CEN X-3 DEDUCED FROM OBSERVATIONS OF ITS ACCRETION WAKE [J].