description NGC 592 Overview
NGC 592 is an H II region in the Triangulum Galaxy, also known as Messier 33 or M33. An H II region is a cloud of ionized hydrogen associated with young, hot stars and ongoing or recent star formation, so NGC 592 is studied as part of the galaxy's population of star-forming nebulae. Heinrich d'Arrest discovered it in 1861, and observations identify an embedded open cluster within the region.
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