ACTIVE GALACTIC NUCLEI FLOW VELOCITIES AND THE HIGHEST ENERGY COSMIC-RAYS

被引：0
|
作者：
QUENBY, JJ [1 ]
DROLIAS, B [1 ]
LIEU, R [1 ]
机构：
[1] UNIV CALIF BERKELEY,CTR EUV ASTROPHYS,BERKELEY,CA 94720
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1994年 / 216卷 / 1-2期
关键词：
D O I：
10.1007/BF00982524
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The dependence of the maximum energy cosmic rays can reach via diffusive shock acceleration in AGN jets on flow speeds is discussed. It is shown that in highly inclined termination shocks where the speed of the de Hoffman-Teller frame is crucial, a good independent knowledge of the jet speed is required to properly assess the extent of the cosmic ray spectrum.
引用
收藏
页码：375 / 378
页数：4
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