Fermi-LAT data reveal GeV gamma-ray emission toward four young massive star clusters, with derived cosmic-ray acceleration efficiencies of order 0.1 to 1 percent of wind power.
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Gamma ray emission from embedded young massive star clusters unveiled by Fermi-LAT
Fermi-LAT data reveal GeV gamma-ray emission toward four young massive star clusters, with derived cosmic-ray acceleration efficiencies of order 0.1 to 1 percent of wind power.