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Apart from the Milky Way, the Large Magellanic Cloud (LMC) is the only othernormal star-forming galaxy that was conclusively detected in high energy (> 100MeV) gamma rays by the Energetic Gamma Ray Telescope (EGRET) on the ComptonGamma-Ray Observatory. However, the sensitivity of EGRET was sufficient only tomarginally resolve the LMC. We report on measurements of the gamma-ray emissionfrom the LMC by the Large Area Telescope (LAT) on the Fermi Gamma-ray SpaceTelescope. For the first time an externally viewed star-forming galaxy is wellresolved in gamma rays. We discuss the distribution of the LMC diffuse emissionas seen by the LAT and implications for cosmic-ray physics.

Fermi LAT Measurements of the Gamma-Ray Emission from the Large Magellanic Cloud