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
收藏
页码：L27 / L30
页数：4
相关论文
共 50 条
12345