The X-Ray Luminosity of FRIs and FRIIs

被引：0
|
作者：
Fan, J. H. [1 ]
Zhang, C. L. [1 ]
Yang, J. H. [2 ]
机构：
[1] Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
[2] Hunan Univ Arts & Sci, Dept Phys & Elect Sci, Changde 415000, Peoples R China
来源：
STARBURST-AGN CONNECTION | 2009年 / 408卷
基金：
中国国家自然科学基金;
关键词：
BL LACERTAE OBJECTS; RADIO GALAXIES; UNIFIED SCHEME;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper, the X-ray data are compiled for the X-ray luminosity calculation for 183 radio galaxies (62 FRIs and 121 FRIIs). We found the averaged X-ray luminosity for FRIs is LogL(X)(1KeV) = 41.84 +/- 3.04erg/s, which is lower than that for FRIIs, which is LogL(X)(1KeV) = 42.43 +/- 1.78erg/s. A K-S test indicates that the two groups have different distribution, implying that the X-ray luminosities of the two groups are different.
引用
收藏
页码：309 / +
页数：3
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