Non-thermal outflows of the Milky Way traced by radio polarization and gamma-ray emission

IF 12.9 1区物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS

Nature Astronomy Pub Date : 2024-09-23 DOI:10.1038/s41550-024-02363-z

引用次数: 0

Abstract

A magnetic halo featuring coherent magnetized ridges several kiloparsecs above and below the Galactic Disk, and a gamma-ray counterpart, are revealed. They probably arise from outflows that are driven by star-forming regions in the Galactic Disk, 3–5 kiloparsecs from the Galactic Centre.

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通过射电偏振和伽马射线发射追踪银河系的非热外流

揭示了一个磁晕，其特点是在银河系盘上下数千帕秒的地方有一条连贯的磁化脊，以及一个伽马射线对应物。它们可能来自银河系盘中恒星形成区的外流，距离银河系中心 3-5 千帕斯卡。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

Nature Astronomy Physics and Astronomy-Astronomy and Astrophysics

CiteScore

19.50

自引率

2.80%

发文量

252

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