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Center-top: supernova remnant in the shape of a flame, many long strands and thin layers of gas that glow orange and blue. Faint gas clouds outline its edges. several scattered blue and red stars surround it. the background is black with small red stars.

DEM L 190

Shreds of the colorful supernova remnant DEM L 190 seem to billow across the screen in this Hubble Space Telescope image. The delicate sheets and intricate filaments are debris from the cataclysmic death of a massive star that once lived in the Large Magellanic Cloud, a small satellite galaxy of the Milky Way. DEM L 190 – also known as LMC N49 – is the brightest supernova remnant in the Large Magellanic Cloud and lies approximately 160,000 light-years away from Earth in the constellation Dorado.

Image Credit: ESA/Hubble & NASA, S. Kulkarni, Y. Chu
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