description HB 21 Overview
HB 21 is a large supernova remnant in the constellation Cygnus, first identified as a radio source in 1953. It is classified as a mixed-morphology remnant, with a shell-like appearance at radio wavelengths and centrally concentrated thermal X-ray emission. Observations indicate interaction between the expanding remnant and nearby molecular clouds, making HB 21 useful for studying how supernova shocks affect dense interstellar gas and produce high-energy radiation.
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