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 | |
刊名 | INTERNATIONAL JOURNAL OF MODERN PHYSICS D |
2003-05 | |
卷号 | 12期号:5页码:781-789 |
关键词 | active galactic nuclei blazars spectral energy distributions |
ISSN号 | 0218-2718 |
通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | 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. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | BL-LACERTAE OBJECTS ; RADIO ; CATALOG ; SCHEME |
收录类别 | SCI |
原文出处 | http://www.worldscientific.com/doi/abs/10.1142/S0218271803003451 |
语种 | 英语 |
WOS记录号 | WOS:000183826000002 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6960] |
专题 | 云南天文台_星系研究组 |
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 |
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.(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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