The optical-X-ray-gamma-ray spectral energy distributions of Gev gamma-ray loud blazars and connection among LBLs, HBLs and FSRQs | |
Xie GZ(谢光中)1,2; Ding SX(丁世学)1,3; Dai H(戴宏)1,2; Liang EW(梁恩维)1,4; Liu HT(刘洪涛)1,5; Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. | |
发表期刊 | INTERNATIONAL JOURNAL OF MODERN PHYSICS D |
2003-05 | |
卷号 | 12期号:5页码:781-789 |
DOI | 10.1142/S0218271803003451 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Active Galactic Nuclei Blazars Spectral Energy Distributions |
摘要 | In this paper, we introduce a new composite spectral indices alpha(gammaxgamma) = alpha(xgamma) - alpha(gamma), and prove alpha(gammaxgamma)(ob) = alpha(xgamma)(ob) - alpha(gamma) = alpha(gammaxgamma)(in), that means alpha(gammaxgamma) is intrinsic. We plot a alpha(xox) - alpha(gammaxgamma) diagram for 25 Gev gamma-ray blazars for which alpha(x) and alpha(gamma) have been provided in the literature, where alpha(xox) = alpha(ox) - alpha(x) which was introduced by Sambruna et al. (1996) and proved that it is intrinsic by our previous paper (Xie et al. 2001). Using this new composite color-color (alpha(xox) - alpha(gammaxgamma)) diagram, we investigated the nature of the HBLsLBLs relationship, and the BL Lacs-FSRQs relationship, in high-energy emission. The results show that the spectral energy distributions of three subclasses of Gev gamma-ray loud blazars axe different, but essentially continuous: HBLs and FSRQs occupy separated regions while LBLs bridge the gap between HBLs and FSRQs. The results are consistent with that derived from a low energy color-color(alpha(xox) - alpha(oro)) diagram by Sambruna et al. (1996) and Xie et al. (2001). However, on the alpha(ox) - alpha(xgamma) diagram, FSRQs, LBLs and HBLs occupy same region. Because both alpha(gammaxgamma) and alpha(xox) are intrinsic, thus, the new connection among HBLs, LBLs and FSRQs obtained by us is intrinsic. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0218-2718 |
URL | 查看原文 |
归档日期 | 2003-08-06 |
WOS记录号 | WOS:000183826000002 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | BL-LACERTAE OBJECTS ; RADIO ; CATALOG ; SCHEME |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6960 |
专题 | 星系研究组 |
通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories, Yunnan Observatory, The Chinese Academy of Sciences, Kunming 650011, China 2.Yunnan Astrophysics Center, Yunan University, Kunming 650091, China 3.Physics Department, Xiangfan University, Xiangfan 441053, China 4.Physics Department, Guangxi University, Nanning 530004, China 5.The Graduate School of the Chinese Academy of Sciences, Beijing, China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Xie GZ,Ding SX,Dai H,et al. The optical-X-ray-gamma-ray spectral energy distributions of Gev gamma-ray loud blazars and connection among LBLs, HBLs and FSRQs[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D,2003,12(5):781-789. |
APA | Xie GZ,Ding SX,Dai H,Liang EW,Liu HT,&Xie, GZ .(2003).The optical-X-ray-gamma-ray spectral energy distributions of Gev gamma-ray loud blazars and connection among LBLs, HBLs and FSRQs.INTERNATIONAL JOURNAL OF MODERN PHYSICS D,12(5),781-789. |
MLA | Xie GZ,et al."The optical-X-ray-gamma-ray spectral energy distributions of Gev gamma-ray loud blazars and connection among LBLs, HBLs and FSRQs".INTERNATIONAL JOURNAL OF MODERN PHYSICS D 12.5(2003):781-789. |
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