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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