DO ULTRAHIGH ENERGY COSMIC RAYS COME FROM ACTIVE GALACTIC NUCLEI AND FERMI gamma-RAY SOURCES? | |
Jiang, Yun-Ying1,2; Hou, L. G.1; Han, J. L.1; Sun, X. H.1; Wang, Wei1 | |
刊名 | ASTROPHYSICAL JOURNAL |
2010-08-10 | |
卷号 | 719期号:1页码:459-468 |
关键词 | cosmic rays galaxies: active magnetic fields methods: statistical |
英文摘要 | We study possible correlations between ultrahigh energy cosmic rays (UHECRs), observed by Auger, AGASA, and Yakutsk, and nearby active galactic nuclei (AGNs) and Fermi sources. We consider the deflection effects by a Galactic magnetic field (GMF) model constrained by the most updated measurements. We found that the average deflection angles of UHECRs by the Galactic magnetic fields are less than 4 degrees. A correlation between the Auger cosmic-ray events and nearby AGNs with a significance level of similar to 4 sigma was found for the Auger UHECR data sets with or without deflection correction. No correlation was found between the AGASA/Yakutsk events with nearby AGNs. Marginal correlations between the Auger events and the Fermi sources, and between AGASA events and Fermi AGNs were found when the deflections calculated by the GMF model were considered. However, no correlation was found between the Yakutsk data and Fermi sources. Some Fermi sources are close to the arrival directions of UHECR events detected by Auger, AGASA, and Yakutsk, most of which are probably chance coincidences rather than objects producing UHECRs in the nearby universe. Four Fermi sources, NGC 4945, ESO 323-G77, NGC 6951, and Cen A, within 100 Mpc have UHECR events within 3 degrees.1 from their positions, which could potentially be cosmic-ray accelerators. However, the association can only be confirmed if more UHECRs are preferably detected in these directions. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000280653100039 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7676] |
专题 | 国家天文台_射电天文研究部 |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China |
推荐引用方式 GB/T 7714 | Jiang, Yun-Ying,Hou, L. G.,Han, J. L.,et al. DO ULTRAHIGH ENERGY COSMIC RAYS COME FROM ACTIVE GALACTIC NUCLEI AND FERMI gamma-RAY SOURCES?[J]. ASTROPHYSICAL JOURNAL,2010,719(1):459-468. |
APA | Jiang, Yun-Ying,Hou, L. G.,Han, J. L.,Sun, X. H.,&Wang, Wei.(2010).DO ULTRAHIGH ENERGY COSMIC RAYS COME FROM ACTIVE GALACTIC NUCLEI AND FERMI gamma-RAY SOURCES?.ASTROPHYSICAL JOURNAL,719(1),459-468. |
MLA | Jiang, Yun-Ying,et al."DO ULTRAHIGH ENERGY COSMIC RAYS COME FROM ACTIVE GALACTIC NUCLEI AND FERMI gamma-RAY SOURCES?".ASTROPHYSICAL JOURNAL 719.1(2010):459-468. |
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