NGC 2122

NGC 2122 is a diffuse nebula and an open cluster in the Large Magellanic Cloud (LMC), visible in the constellation Mensa. It was discovered by James Dunlop in 1826.

The nebula, N180B, is an active star-forming region, containing some of the brightest known clusters. These clusters are known as OB associations because they are formed by hot stars of spectral type O and B. The stars of type O are very luminous and have incredibly strong stellar winds. These stellar winds have the ability to drain the gas over hundreds of light years, forming thick clouds of dust, both of which are evident in N180B. Think of it as a new star-forming region and there has never been a supernova explosion.

N180B is an H II region (ionized hydrogen gas region). There are 100-year-long light streamers of dust that run along the H II region, according to smaller dust clouds. If the pressure of the interstellar gas is high, the star formation could take place in these small clouds of dust.

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