High-energy neutrinos present the ultimate signature for a cosmic ray accelerator. Galactic sources responsible for acceleration of cosmic ray up to the knee in cosmic ray spectrum will provide a guaranteed, albeit subdominant, contribution to the high-energy cosmic neutrino flux. In this review, we discuss the the prospects for identification of high-energy neutrinos from sources of the very high energy gamma ray emission in the Milky Way. We present the status of the search for point-like and extended emission from these sources, and describe how the results of these studies indicate that neutrino telescopes are closing in on identifying Galactic sources of high-energy neutrinos.

中文翻译：

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确定高能中微子的银河来源

高能中微子是宇宙射线加速器的终极特征。负责在宇宙射线光谱中将宇宙射线加速到膝部的银河源将为高能宇宙中微子通量提供有保证的贡献，尽管是次要的。在这篇综述中，我们讨论了从银河系中超高能伽马射线发射源中识别高能中微子的前景。我们介绍了从这些来源寻找点状和扩展发射的状态，并描述了这些研究的结果如何表明中微子望远镜正在接近识别高能中微子的银河源。