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000293196 1001_ $$0P:(DE-H253)PIP1021898$$aOhm, Stefan$$b0$$eCorresponding author
000293196 245__ $$aThe exceptionally powerful TeV $\gamma$-ray emitters in the Large Magellanic Cloud
000293196 260__ $$aWashington, DC [u.a.]$$bAmerican Association for the Advancement of Science16205$$c2015
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000293196 520__ $$aThe Large Magellanic Cloud, a satellite galaxy of the Milky Way, has been observed with the High Energy Stereoscopic System (H.E.S.S.) above an energy of 100 billion electron volts for a deep exposure of 210 hours. Three sources of different types were detected: the pulsar wind nebula of the most energetic pulsar known, N 157B; the radio-loud supernova remnant N 132D; and the largest nonthermal x-ray shell, the superbubble 30 Dor C. The unique object SN 1987A is, unexpectedly, not detected, which constrains the theoretical framework of particle acceleration in very young supernova remnants. These detections reveal the most energetic tip of a γ-ray source population in an external galaxy and provide via 30 Dor C the unambiguous detection of γ-ray emission from a superbubble.
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000293196 536__ $$0G:(EU-Grant)259391$$aP-WIND - New light on the gamma-ray sky: unveiling cosmic-ray accelerators in the Milky Way and their relation to pulsar wind nebulae (259391)$$c259391$$fERC-2010-StG_20091028$$x1
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000293196 7001_ $$0P:(DE-H253)PIP1004231$$aKlepser, Stefan$$b1
000293196 7001_ $$0P:(DE-H253)PIP1015478$$aStegmann, Christian$$b2
000293196 7001_ $$0P:(DE-HGF)0$$aH.E.S.S. Collaboration$$b3$$eCollaboration author
000293196 773__ $$0PERI:(DE-600)2066996-3$$a10.1126/science.1261313$$gVol. 347, no. 6220, p. 406 - 412$$n6220$$p406 - 412$$tScience$$v347$$x1095-9203$$y2015
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