...
机译:活性银核的隐藏核心作为中型中微子的起源:与MEV伽马射线连接的关键测试
Penn State Univ Dept Phys University Pk PA 16802 USA|Penn State Univ Dept Astron & Astrophys University Pk PA 16802 USA|Penn State Univ Inst Gravitat & Cosmos Ctr Multimessenger Astrophys University Pk PA 16802 USA|Yukawa Inst Theoret Phys Kyoto Kyoto 6068502 Japan;
Penn State Univ Dept Phys University Pk PA 16802 USA|Penn State Univ Dept Astron & Astrophys University Pk PA 16802 USA|Penn State Univ Inst Gravitat & Cosmos Ctr Multimessenger Astrophys University Pk PA 16802 USA;
Penn State Univ Dept Phys University Pk PA 16802 USA|Penn State Univ Dept Astron & Astrophys University Pk PA 16802 USA|Penn State Univ Inst Gravitat & Cosmos Ctr Multimessenger Astrophys University Pk PA 16802 USA;
机译:活性银河系核的宇宙MeV伽玛射线背景和X射线硬光谱:对热银冠冕起源的启示
机译:活性银河核的宇宙MeV伽玛射线背景和X射线硬光谱:对热银冠冕起源的启示
机译:未来的MeV伽马射线活跃银河核种群研究前景
机译:多普勒促进伽马射线爆发和活性银核的喷射辐射效果
机译:活跃银河核扩散中微子发射的上限。
机译:活跃的银河核
机译:活性银核的隐藏核心作为中型中微子的起源:与MEV伽马射线连接的关键测试