description N49 (LMC) Overview
N49 is a supernova remnant in the Large Magellanic Cloud, a satellite galaxy of the Milky Way located in the southern sky. Its expanding shock structure is asymmetric and filamentary, and the remnant is associated with the soft gamma repeater SGR 0526-66, a source of recurring high-energy gamma-ray activity. N49 is studied through observations at X-ray and other wavelengths.
help N49 (LMC) FAQ
What is N49?
N49 is a supernova remnant in the Large Magellanic Cloud. It is an expanding cloud of shock-heated material left by a stellar explosion.
Where is N49 located?
N49 is in the Large Magellanic Cloud, a satellite galaxy of the Milky Way in the southern sky. Its location makes it an important object for studying supernova remnants beyond our own galaxy.
Why is SGR 0526-66 associated with N49?
N49 is associated with the soft gamma repeater SGR 0526-66. That source produces recurring bursts of high-energy radiation and is linked to the remnant's scientific interest.
What does N49 look like?
Its expanding shock structure is asymmetric and filamentary. Those uneven strands trace material and shock fronts produced by the original stellar explosion.
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