Mechanism of very high-energy radiation in BL Lacertae object 3C 66A
文献类型:期刊论文
作者 | Yang JP(杨建平)1,2,3![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
![]() |
出版日期 | 2010-02 |
卷号 | 511 |
关键词 | BL Lacertae objects: individual: 3C 66A |
ISSN号 | 0004-6361 |
产权排序 | 第一完成单位 |
通讯作者 | Yang, J (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
英文摘要 | Aims. Our goal is to understand the nature of blazars and the mechanisms for generating high-energy.-rays, through investigation of the blazar 3C 66A. Methods. We model the high-energy spectrum of 3C 66A, which was observed recently with the Fermi-LAT and VERITAS telescopes. The spectrum has a hard change from the energy range of 0.2-100 GeV to 200-500 GeV in recent almost contemporaneous observations of two telescopes. Results. The de-absorbed VERITAS spectrum depends strongly on redshift, which is highly uncertain. If z = 0.444 is adopted, we are able to use the SSC model to produce the Fermi-LAT component and the EC model to the VERITAS component. However, if z = 0.1, the intrinsic VERITAS spectrum will be softer, and there will be a smooth link between the Fermi-LAT and VERITAS spectra that can be explained using an SSC model. |
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 GALACTIC NUCLEI ; RAY BRIGHT BLAZARS ; TEV BLAZARS ; GAMMA-RAYS ; PARTICLE-ACCELERATION ; RELATIVISTIC JETS ; WEBT CAMPAIGN ; EMISSION ; 3C-66A ; VARIABILITY |
收录类别 | SCI ; EI |
原文出处 | http://www.aanda.org/articles/aa/abs/2010/03/aa13035-09/aa13035-09.html |
语种 | 英语 |
WOS记录号 | WOS:000275752400011 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4999] ![]() |
专题 | 云南天文台_高能天体物理研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.National Astronomical Observatories, Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, PR China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, PR China 3.Yunnan Agricultural University, Kunming 650201, PR China |
推荐引用方式 GB/T 7714 | Yang JP,Wang JC. Mechanism of very high-energy radiation in BL Lacertae object 3C 66A[J]. ASTRONOMY & ASTROPHYSICS,2010,511. |
APA | Yang JP,&Wang JC.(2010).Mechanism of very high-energy radiation in BL Lacertae object 3C 66A.ASTRONOMY & ASTROPHYSICS,511. |
MLA | Yang JP,et al."Mechanism of very high-energy radiation in BL Lacertae object 3C 66A".ASTRONOMY & ASTROPHYSICS 511(2010). |
入库方式: OAI收割
来源:云南天文台
浏览0
下载0
收藏0
其他版本
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。