description DWB 175 Overview
DWB 175 is an optically visible H II region in the Cygnus X star-forming complex, a designation used for ionized gas associated with star formation. The name comes from Dickel, Wendker, and Bieritz, whose 1969 catalog surveyed H II regions in Cygnus X. DWB 175 is described as the smaller lower-left portion of the Sh2-112 nebular field and is discussed in connection with young stellar objects identified in multiwavelength studies.
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