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

被引:0
|
作者
Zhang, He-Shou [1 ]
Carretti, Ettore [2 ]
Ponti, Gabriele [1 ]
机构
[1] INAF Osservatorio Astron Brera, Merate, Italy
[2] INAF Ist Radioastron, Bologna, Italy
来源
关键词
X-RAY;
D O I
10.1038/s41550-024-02363-z
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:1357 / 1358
页数:2
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