EVIDENCE FOR A SECOND COMPONENT IN THE HIGH-ENERGY CORE EMISSION FROM CENTAURUS A? | |
Sahakyan, N.1,2; Yang, R.3; Aharonian, F. A.4; Rieger, F. M.5 | |
刊名 | ASTROPHYSICAL JOURNAL LETTERS |
2013-06-10 | |
卷号 | 770期号:1页码:0 |
关键词 | galaxies: active galaxies: individual (Cen A) |
ISSN号 | 2041-8205 |
通讯作者 | Sahakyan, N (reprint author), ICRANet, Piazz Repubbl 10, I-65122 Pescara, Italy. Email: 0 |
英文摘要 | We report on an analysis of Fermi Large Area Telescope data from four years of observations of the nearby radio galaxy Centaurus A (Cen A). The increased photon statistics results in a detection of high-energy (>100 MeV) gamma-rays up to 50 GeV from the core of Cen A, with a detection significance of about 44 sigma. The average gamma-ray spectrum of the core reveals evidence for a possible deviation from a simple power law. A likelihood analysis with a broken power-law model shows that the photon index becomes harder above E-b similar or equal to 4 GeV, changing from Gamma(1) = 2.74 +/- 0.03 below to Gamma(2) = 2.09 +/- 0.20 above. This hardening could be caused by the contribution of an additional high-energy component beyond the common synchrotron self-Compton jet emission. No clear evidence for variability in the high-energy domain is seen. We compare our results with the spectrum reported by H.E.S.S. in the TeV energy range and discuss possible origins of the hardening observed. |
学科主题 | Physics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | LARGE-AREA TELESCOPE ; GAMMA-RAY EMISSION ; RADIO GALAXY CENTAURUS ; BLACK-HOLE ; NGC 5128 ; JET ; RADIATION ; CATALOG ; M87 |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000319723500006 |
公开日期 | 2014-01-08 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/9768] |
专题 | 紫金山天文台_暗物质和空间天文实验室 |
作者单位 | 1.ICRANet, I-65122 Pescara, Italy 2.NAS Armenia, Inst Phys Res, Ashtarak 2, Armenia 3.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210008, Peoples R China 4.Dublin Inst Adv Studies, Dublin 2, Ireland 5.Max Planck Inst Kernphys, D-69029 Heidelberg, Germany |
推荐引用方式 GB/T 7714 | Sahakyan, N.,Yang, R.,Aharonian, F. A.,et al. EVIDENCE FOR A SECOND COMPONENT IN THE HIGH-ENERGY CORE EMISSION FROM CENTAURUS A?[J]. ASTROPHYSICAL JOURNAL LETTERS,2013,770(1):0. |
APA | Sahakyan, N.,Yang, R.,Aharonian, F. A.,&Rieger, F. M..(2013).EVIDENCE FOR A SECOND COMPONENT IN THE HIGH-ENERGY CORE EMISSION FROM CENTAURUS A?.ASTROPHYSICAL JOURNAL LETTERS,770(1),0. |
MLA | Sahakyan, N.,et al."EVIDENCE FOR A SECOND COMPONENT IN THE HIGH-ENERGY CORE EMISSION FROM CENTAURUS A?".ASTROPHYSICAL JOURNAL LETTERS 770.1(2013):0. |
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