I point out a correlation between gamma-ray emissivity and the historical star formation rate in the Large Magellanic Cloud ~12.5 Myr ago. This correlation bolsters the view that CRs in the LMC are accelerated by conglomerations of supernova remnants: i.e. superbubbles and supergiant shells.
CCD SDSS gr photometry of poorly studied star clusters in the Large Magellanic Cloud
Spatial variations of dust abundances across the Large Magellanic Cloud
Young stars in the periphery of the Large Magellanic Cloud
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