Gamma-ray emission from the gamma-ray-loud BL Lac objects | |
Xie GZ(谢光中)1,2,3,4; Dai BZ(戴本忠)1,3; Liang EW(梁恩维)1,2,5; Xie, ZH6; Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China. | |
发表期刊 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS |
2001-12 | |
卷号 | 1期号:6页码:494-500 |
DOI | 10.1088/1009-9271/1/6/494 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Gamma Rays Bl Lacertae Objects : General |
摘要 | Using the HST observation data of BL Lac objects by Urry et al. and gamma-ray observation data, we find that there is a correlation between Fgamma and F-O(nuclei) for gamma-ray-loud BL Lac objects (correlation coefficients: gamma = 0.63, p = 4.0 x 10(-2)), but no correlation between F-gamma and F-O(host), where F-O(nuclei) and F-O(host) are the fluxes of nuclei and host galaxy in V-band. For 19 gamma-ray-loud BL Lac objects with observed spectral index in multi-wavebands, the spectral index correlations between any two bands are as follow: (1) there is a strong correlation between alpha(gamma) and alpha(K) for 15 BL Lac objects (gamma = 0.84, p = 3.11 x 10(-4)); (2) the correlation between alpha(gamma) and alpha(O) for 12 BL Lac objects is gamma = 0.82, p = 1.5 x 10(-3); (3) there is no correlation between alpha(gamma), and alpha(x) for 16 BL Lac objects. The results, together with characteristic double-humped shape of their SEDs, show that the synchrotron self-Compton mechanism might be a main mechanism for the gamma-ray emission of the BL Lac objects. The electrons emitting IR and optical radiation via synchrotron are also responsible for upscattering these photons to gamma-rays, and a variability in IR-optical regime should be accompanied by a change in the gamma-rays. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 1009-9271 |
URL | 查看原文 |
归档日期 | 2002-02-27 |
WOS记录号 | WOS:000173057800003 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | ACTIVE GALAXY MARKARIAN-421 ; NEAR-INFRARED EMISSION ; LACERTAE OBJECTS ; GALACTIC NUCLEI ; TEV PHOTONS ; BLAZARS ; SPECTRA ; MODEL ; PKS-2155-304 ; PHOTOMETRY |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6932 |
专题 | 星系研究组 |
通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.Yunnan Astronomical Observatory, Chinese Academy of Science, Kunming 650011 2.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 3.Yunnan Astrophysics Center, Yunnan University, Kunming 650091 4.United Laboratory of Optical Astronomy, Chinese Academy of Sciences 5.Department of Physics, Guangxi University, Nanning 530004 6.Department of Physics, University of Hong Kong |
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,Dai BZ,Liang EW,et al. Gamma-ray emission from the gamma-ray-loud BL Lac objects[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2001,1(6):494-500. |
APA | Xie GZ,Dai BZ,Liang EW,Xie, ZH,&Xie, GZ .(2001).Gamma-ray emission from the gamma-ray-loud BL Lac objects.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,1(6),494-500. |
MLA | Xie GZ,et al."Gamma-ray emission from the gamma-ray-loud BL Lac objects".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 1.6(2001):494-500. |
条目包含的文件 | ||||||
文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Gamma-ray Emission f(232KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论