TeV耀变体
TeV blazar
查看参考文献142篇
文摘
|
地面切仑科夫望远镜阵列(IACTs)与空间费米大面积望远镜(Fermi-LAT)的协同观测, 推动了耀变体高能辐射的研究, 特别在耀变体的宽线区结构(BLR)、喷流的物质组成、粒子加速、辐射过程、以及高能宇宙射线起源等方面取得新进展. 同时, 耀变体产生的TeV伽马射线和极高能粒子在传播过程中会与河外背景光(EBL)、微波背景(CMB)及星际磁场(IGMF)发生作用, 可以用TeV耀变体研究河外背景光及星际磁场的强度,以及它对宇宙学的影响. 本文中, 我们简要介绍了TeV耀变体的观测设备、统计性质和相关的研究进展等内容. |
其他语种文摘
|
The observation from the ground-based Imaging Atmospheric Cherenkov Telescope arrays (IACTs) and Fermi Large Area Telescope (Fermi-LAT), prompts significantly the study on the high-energy emission in blazars. They involve the structure of the Broad-Line Region (BLR), the content of the jet, particle acceleration, radiation processes, as well as the origin of the high-energy cosmic rays in blazars etc. Based on the interaction of the TeV gamma rays and ultra-high-energy particles from blazars with the Extragalactic Background Light (EBL), Microwave Background (CMB) and Intergalactic Magnetic Field (IGMF), we can explore EBL, CMB and IGMF, as well as the cosmological impact of blazars. In the paper, we introduce briefly the gamma-ray observation equipment, statistical properties and study progresses in TeV blazars. |
来源
|
中国科学. 物理学
, 力学, 天文学,2015,45(11):119506-1-119506-21 【核心库】
|
DOI
|
10.1360/sspma2015-00272
|
关键词
|
耀变体
;
TeV伽马射线
;
高能宇宙射线
|
地址
|
中国科学院云南天文台, 昆明, 650011
|
语种
|
中文 |
文献类型
|
综述型 |
ISSN
|
1674-7275 |
学科
|
天文学 |
基金
|
国家自然科学基金
;
中国科学院先导B专项
|
文献收藏号
|
CSCD:5549363
|
参考文献 共
142
共8页
|
1.
Urry C M. Unified schemes for radio-loud active galactic nuclei.
Publ Astron Soc Pac,1995,107:803-845
|
CSCD被引
171
次
|
|
|
|
2.
Stocke J T. Broad Lyα emission from three nearby BL lacertae objects.
Astrophys J,2011,732:113-121
|
CSCD被引
4
次
|
|
|
|
3.
Abdo A A. The spectral energy distribution of Fermi bright blazars.
Astrophys J,2010,716:30-70
|
CSCD被引
61
次
|
|
|
|
4.
Finke J D. Synchrotron self-compton analysis of TeV X-ray-selected BL lacertae objects.
Astrophys J,2008,686:181-194
|
CSCD被引
8
次
|
|
|
|
5.
Dermer C D. Gamma-ray studies of blazars:Synchro-compton analysis of flat spectrum radio quasars.
Astrophys J,2009,692:32-46
|
CSCD被引
6
次
|
|
|
|
6.
Dermer C D. High-energy gamma radiation from extragalactic radio sources.
Astron Astrophys,1993,256:27-30
|
CSCD被引
1
次
|
|
|
|
7.
Dermer C D. Model for the high-energy emission from blazars.
Astrophys J,1993,416:458-484
|
CSCD被引
25
次
|
|
|
|
8.
Sikora M. Comptonization of diffuse ambient radiation by a relativistic jet:The source of gamma rays from blazars?.
Astrophys J,1994,421:153-162
|
CSCD被引
44
次
|
|
|
|
9.
Donea A C. Radiation fields of disk, BLR and torus in quasars and blazars:Implications for γ-ray absorption.
Astropart Phys,2003,18:377-393
|
CSCD被引
3
次
|
|
|
|
10.
Liu H T. Absorption of 10-200 GeV gamma rays by radiation from broad-line regions in blazars.
Astrophys J,2006,653:1089-1097
|
CSCD被引
5
次
|
|
|
|
11.
Celotti A. Bulk comptonization spectra in blazars.
Mon Not R Astron Soc,2007,375:417-424
|
CSCD被引
1
次
|
|
|
|
12.
Ghisellini G. The blazar sequence:A new perspective.
Mon Not R Astron Soc,2008,387:1669-1680
|
CSCD被引
12
次
|
|
|
|
13.
Ghisellini G. Canonical high-power blazars.
Mon Not R Astron Soc,2009,397:985-1002
|
CSCD被引
17
次
|
|
|
|
14.
Lei M. The effect of the broad-line region with geometrical structures on gamma-ray absorption in blazars.
Publ Astron Soc Jpn,2014,66:7-14
|
CSCD被引
1
次
|
|
|
|
15.
Blazejowski M. Comptonization of infrared radiation from hot dust by relativistic jets in quasars.
Astrophys J,2000,545:107-116
|
CSCD被引
14
次
|
|
|
|
16.
Mucke A. A proton synchrotron blazar model for flaring in Markarian 501.
Astropart Phys,2001,15:121-136
|
CSCD被引
5
次
|
|
|
|
17.
Bottcher M. Leptonic and hadronic modeling of Fermi-detected blazars.
Astrophys J,2013,768:54-68
|
CSCD被引
11
次
|
|
|
|
18.
Cerruti M. A hadronic origin for ultra-high-frequency-peaked BL lac objects.
Mon Not R Astron Soc,2015,448:910-927
|
CSCD被引
6
次
|
|
|
|
19.
Petropoulou M. Bethe-Heitler emission in BL lacs:Filling the gap between X-rays and γ-rays.
Mon Not R Astron Soc,2015,447:36-48
|
CSCD被引
1
次
|
|
|
|
20.
Atwood W B. The large area telescope on the Fermi gamma-ray space telescope mission.
Astrophys J,2009,697:1071-1102
|
CSCD被引
71
次
|
|
|
|
|