The contribution of winds from star clusters to the Galactic cosmic-ray population

LEO's

Nature Astronomy, Published online: 09 January 2024; doi:10.1038/s41550-023-02168-6

High-energy radiation originating in the wind termination shock of young star clusters has been observed, without contamination from other sources such as supernovae. This adds the winds of star clusters to the list of cosmic-ray accelerators within the Galaxy.

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