On the anisotropy of E _0 ≥ 5.5× 10 ~(19) eV cosmic rays according to data of the Pierre Auger Collaboration

Glushkov A.V.

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On the anisotropy of E _0 ≥ 5.5× 10 ~(19) eV cosmic rays according to data of the Pierre Auger Collaboration

机译：根据Pierre Auger协作的数据，关于E _0≥5.5×10〜（19）eV宇宙射线的各向异性

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The Pierre Auger Collaboration discovered, in a solid angle of radius about 18°, a local group of cosmic rays having energies in the region E _0 ≥ 5.5 × 10 ~(19) eV and coming from the region of the Gen A radio galaxy, whose galactic coordinates are l _G = 309.5° and b _G = 19.4°. Near it, there is the Centaur supercluster of galaxies, its galactic coordinates being l _G = 302.4° and b _G = 21.6°. It is noteworthy that the Great Attractor, which may have a direct bearing on the observed picture, is also there.

机译：皮埃尔·奥格（Pierre Auger）合作社在半径约为18°的立体角中发现了一组宇宙射线，这些宇宙射线的能量在E _0≥5.5×10〜（19）eV范围内，并且来自Gen A射电星系的区域，其银河坐标为l _G = 309.5°和b _G = 19.4°。在它附近，有半人马座星系超级星团，其银河坐标为l _G = 302.4°和b _G = 21.6°。值得注意的是，也可能与观察到的图像有直接关系的Great Attractor也在那里。

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《Physics of atomic nuclei》 |2012年第2期|共6页
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Glushkov A.V.;
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1. On the anisotropy of E _0 ≥ 5.5× 10 ~(19) eV cosmic rays according to data of the Pierre Auger Collaboration [J] . Glushkov A.V. Physics of atomic nuclei . 2012,第2期

机译：根据Pierre Auger协作的数据，关于E _0≥5.5×10〜（19）eV宇宙射线的各向异性
2. Upper limit on the cosmic-ray photon flux above 10(19) eV using the surface detector of the Pierre Auger Observatory [J] . Abraham J, Abreu P, Aglietta M, Astroparticle physics . 2008,第4期

机译：使用Pierre Auger天文台的表面检测器，对宇宙射线光子通量的上限高于10（19）eV
3. An upper limit to the photon fraction in cosmic rays above 10(19) eV from the Pierre Auger Observatory [J] . Abraham J, Aglietta M, Aguirre C, Astroparticle physics . 2007,第2a3期

机译：皮埃尔·奥格天文台的宇宙射线中高于10（19）eV的光子分数的上限
4. Large-Scale Distribution of Arrival Directions of Cosmic Rays Detected at the Pierre Auger Observatory Above 10 PeV [C] . Olivier Deligny, Pierre Auger Collaboration Cosmic Ray Anisotropy Workshop . 2014

机译：在10 PEV以上的Pierre Auger观测台检测到宇宙射线到达方向的大规模分布
5. Small scale angular clustering of the highest energy cosmic rays in the surface detector data of the Pierre Auger Cosmic Ray Observatory. [D] . Ohnuki, Tohru. 2005

机译：皮埃尔·奥格宇宙射线天文台的表面探测器数据中最高能量宇宙射线的小规模角聚类。
6. Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory [O] . A. Aab, P. Abreu, M. Aglietta, -1

机译：在Pierre Auger天文台将宇宙射线能量和到达方向结合起来以寻找模式
7. On the Anisotropy of E0 >= 5.5$ imes$1019 eV Cosmic Rays according to Data of the Pierre Auger Collaboration [O] . Glushkov, A. V. 2012

机译：关于各向异性的E0> = 5.5 $ \倍1019美元eV宇宙射线根据 pierre auger Collaboration的数据
8. Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of 10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array. [R] . Aab, A. 2014

机译：搜索在皮埃尔奥格天文台和望远镜阵列上检测到的能量为10 ^ {19} $ eV的宇宙射线到达方向的大尺度各向异性。

On the anisotropy of E _0 ≥ 5.5× 10 ~(19) eV cosmic rays according to data of the Pierre Auger Collaboration

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