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NGC 346 is a planetary nebula located within the Small Magellanic Cloud. It’s recognized as the most luminous star-forming region of this satellite galaxy and contains a dense cluster of young, hot stars. This emission nebula, fueled by the remnants of a massive star, provides valuable insights for...
E0102-72.3 is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. It is the result of a massive star's core collapse that occurred roughly 2,000 years ago as observed from Earth. The remnant is scientifically significant because its ex...
NGC 602 is an emission nebula located within the Small Magellanic Cloud. It represents a young star cluster actively forming new stars under conditions of extremely low metal content—significantly less heavy elements than found in our own Milky Way. This makes it valuable for astronomers studying ea...
NGC 371 is an open star cluster associated with an emission nebula, located within the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. The cluster is notable for containing a high concentration of massive, variable supergiant stars, which actively contribute to the surrounding H II re...
NGC 248 is an emission nebula and star-forming region in the Small Magellanic Cloud, a dwarf satellite galaxy of the Milky Way. It contains glowing hydrogen gas ionized by radiation from young, massive stars and is classified as an H II region. Scottish astronomer James Dunlop recorded the object in...
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