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Fermi-LAT study of diffuse gamma-ray emission in the outer Galaxy and implications for Galactic cosmic-rays

机译:Fermi-LAT研究外银河中的弥散伽马射线发射及其对银河系宇宙射线的影响

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摘要

Galactic diffuse r-ray emission is a powerful probe to study cosmic rays and the interstellar medium in distant locations. We analyzed the interstellar r-ray emission from the outer Galaxy measured by the Large Area Telescope (LAT) on board Fermi [1, 2]. The r-ray emissivity as a function of Galactocentric distance does not show a significant gradient beyond the solar circle, indicating larger cosmic-ray densities than what has been usually assumed so far. We report the analysis and discuss their implications for the origin and propagation of Galactic cosmic rays.
机译:银河漫射r射线发射是研究遥远位置的宇宙射线和星际介质的有力探针。我们分析了费米[1,2]板上大面积望远镜(LAT)测得的外星系的星际r射线发射。 r射线发射率与半轴距的关系没有显示出太阳圆以外的明显梯度,这表明宇宙射线的密度比迄今通常假定的更大。我们报告分析并讨论它们对银河系宇宙射线的起源和传播的影响。

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