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LMC N49
N49 or LMC N49〔 (PKS 0525-66,〔〔 PKS B0525-661,〔 PKS J0525-6604,〔 SNR J052559-660453〔) is the brightest supernova remnant in the Large Magellanic Cloud, approximately 160,000 light-years from Earth. It has been assessed to be roughly 5,000 years old.〔 The latest pictures of N49 by the Chandra X-ray Observatory have revealed a bullet-shaped object traveling at about 5 million miles an hour away from a bright X-ray and gamma-ray point source, probably a neutron star with an extremely powerful magnetic field, known as a soft gamma repeater.〔 A particularly strong gamma-ray burst from LMC N49 was detected on March 5, 1979.〔 ==References==
* Harvard-Smithsonian Center for Astrophysics, ("N49: A supernova remnant in the Large Magellanic Cloud" )
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