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机译:AKARI观测到尘埃星系的无线电发射
~2.2, which is consistent with the previous measurements from the literature.
〜2.2,与文献中先前的测量结果一致。
The Astronomical Observatory of the Jagiellonian University, ul. Orla 171, 30-244 Krakow, Poland;
The Astronomical Observatory of the Jagiellonian University, ul. Orla 171, 30-244 Krakow, Poland,National Centre for Nuclear Research, ul. Hoza 69, 00-681 Warszawa, Poland;
Department of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, 464-8602 Nagoya, Japan;
Department of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, 464-8602 Nagoya, Japan;
The Astronomical Observatory of the Jagiellonian University, ul. Orla 171, 30-244 Krakow, Poland;
Galaxies; Dust; AGNs; Radio-infrared correlation;
机译:来自Akari全天调查的局部尘土飞扬星系和尘土飞扬AGN的无线电红外相关
机译:尘埃形成星系的微波和无线电发射:对宇宙无线电背景的影响
机译:AKARI检测发光红外星系中的热尘-搜索尘埃活跃的银河核
机译:活跃的星系直播的地方:Akari-nep字段中的无线电agn的一片全景视图
机译:辐射晕,宇宙射线电子传播和热电离介质的特性,是通过观测银河系和边缘螺旋星系中的无线电同步加速器发射而确定的。
机译:关于银河系和其他星系的非热辐射发射光谱
机译:来自Akari全天调查的局部尘土飞扬星系和尘土飞扬AGN的无线电红外相关
机译:用Fermi-LaT观测的宽带无线电星系:GeV(γ) - 辐射的起源。