HIGH-ENERGY GAMMA-RADIATION FROM EXTRAGALACTIC RADIO-SOURCES

被引：0

作者：

DERMER, CD

SCHLICKEISER, R

MASTICHIADIS, A

机构：

[1] MAX PLANCK INST RADIOASTRON, HUGEL 69, W-5300 BONN 1, GERMANY

[2] RICE UNIV, DEPT SPACE PHYS & ASTRON, HOUSTON, TX 77251 USA

[3] MAX PLANCK INST NUCL PHYS, W-6900 HEIDELBERG 1, GERMANY

来源：

ASTRONOMY & ASTROPHYSICS | 1992年 / 256卷 / 02期

关键词：

GAMMA RAYS; EXTRAGALACTIC RADIO SOURCES; INVERSE COMPTON SCATTERING; 3C273; 3C279;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We propose that the important relationship between 3C 273 and 3C 279, the first two extragalactic sources detected at > 100 MeV energies, is their superluminal nature. In support of this conjecture, we propose a kinematic focusing mechanism, based on Compton scattering of accretion-disk photons by relativistic nonthermal electrons in the jet, that preferentially emits gamma rays in the superluminal direction.

引用

页码：L27 / L30

页数：4

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