A TWO-COMPONENT POWER LAW COVERING NEARLY FOUR ORDERS OF MAGNITUDE IN THE POWER SPECTRUM OFSPITZERFAR-INFRARED EMISSION FROM THE LARGE MAGELLANIC CLOUD
A TWO-COMPONENT POWER LAW COVERING NEARLY FOUR ORDERS OF MAGNITUDE IN THE POWER SPECTRUM OFSPITZERFAR-INFRARED EMISSION FROM THE LARGE MAGELLANIC CLOUD
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