Gamma-ray emission from the gamma-ray-loud BL Lac objects
文献类型：期刊论文
| 作者 | 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
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| 刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
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| 出版日期 | 2001-12 |
| 卷号 | 1期号:6页码:494-500 |
| 关键词 | gamma rays BL Lacertae objects : general |
| ISSN号 | 1009-9271 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | 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. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | 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 |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/1009-9271/1/6/494/ |
| 语种 | 英语 |
| WOS记录号 | WOS:000173057800003 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6932]  |
| 专题 | 云南天文台_星系研究组 |
| 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 |
| 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.(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. |
入库方式： OAI收割
来源：云南天文台
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