射电星系

活动星系核分为类星体，塞弗特星系，射电星系，Blazar，Liner等。

The active galactic nucleus divides into QSO , Seyfert galaxies , radio galaxy , Blazar , Liner and so on .

这种相对论性快电子分布等离子体的色散关系能为解释星系核、射电星系和类星体电磁辐射方面的问题提供理论参考。其次，本文研究了修正的kappa分布等离子体横振荡的色散关系。

The dispersion relations of the relativistic plasma with fast electron distribution is significative to study the electromagnetic radiation of the galactic nucleus , the radio galaxy and the quasars . Second , the dispersion relation for electromagnetic oscillation in relativistic plasma with a modified kappa distribution is investigated .

射电星系X射线喷流的观测等。

The X-ray jets identified by Chandra observations .

11个类星体、3个BLLac天体和1个射电星系的Υ射线辐射已得到证认。

Gamma-ray emissions from 11 quasars , 3 BL Lac Objects and 1 radiogalaxy have been identified .

双源射电星系的演化特性

Some characteristics in evolution of radio galaxies with double structure

一个射电星系与之有关，但是它比类星体要大。

A radio galaxy is related to , but appears larger than , a quasar .

喷流结构普遍存在于活动星系核尤其是射电星系和类星体当中。

Jets commonly exist in the active galactic nuclei , especially in radio galaxies and QSOs .

γ爆与星系群、星系对及射电星系的交叉相关分析

The Cross-Correlations of Gamma-Ray Bursts with Groups of Galaxies , Isolated Pairs of Galaxies and Radio Galaxies

射电星系的统计研究

Statistic research of radio galaxies

近年来通过对微波背景辐射及遥远射电星系发出的射电波的观测表明，它们存在一与地球运动相关的各向异性。

Recent observations on microwave background radiation and distribution of distant radio galaxies demonstrate that there exists dipole anisotropy in relation to the motion of the Earth .

开展这些亮而远的射电星系研究有助于我们了解早期宇宙的演化以及星系活动的内在原因。

The study of such luminous and distant radio galaxies will be helpful to the exploration of the early universe and to the knowledge about the intrinsic cause of the galaxy activity .

最近的工作重点考查这一类型的星系：星系中具有类似木星一样的巨形气态行星.一个射电星系与之有关，但是它比类星体要大。

The latest work focuses on a type of star system that contains gas giants known as hot Jupiters . A radio galaxy is related to , but appears larger than , a quasar .

本篇论文主要对射电强活动星系核的中央引擎和射电喷流的性质进行了一些研究。

In this thesis , we present the studies of the central engine and radio jets in radio-loud Active Galaxies Nuclei .