RCW 140 vs IC 1848
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RCW 140
RCW 140, also catalogued as Sh 2-19, is an emission nebula and H II region in the direction of Sagittarius. An H II region is a cloud of ionized hydrogen surrounding or near hot, young stars. Infrared sources associated with RCW 140 have been studied in connection with star formation, because infrared observations can reveal young stellar objects and dense material hidden by interstellar dust.
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IC 1848
IC 1848, commonly known as the Soul Nebula, is an emission nebula in the constellation Cassiopeia, approximately 7,500 light-years from Earth. The nebula spans about 150 light-years and consists of ionized hydrogen gas excited by radiation from embedded young stars. IC 1848 is often studied alongside its neighbor IC 1805 (the Heart Nebula), as both are part of the same complex of star-forming regi...
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