description HB 3 (G132.7+1.3) Overview
HB 3, also designated G132.7+1.3, is an evolved, faint shell-type supernova remnant in the direction of the constellation Cassiopeia. Radio surveys place it next to the W3, W4, and W5 star-forming complex, and studies have examined evidence that the remnant is interacting with molecular material associated with the W3 H II region. It is of interest to astronomers studying how an old supernova remnant affects nearby interstellar clouds.
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