description Sh2-106 Overview
Sh2-106, also called Sharpless 2-106, is a compact bipolar emission nebula and star-forming region in the constellation Cygnus. Its two lobes of glowing gas are separated by a dark lane of dust, producing a pronounced hourglass appearance. The structure is shaped by energetic outflows and radiation from S106 IR, a massive young star embedded near the nebula's center, making the object useful for studying the early evolution of high-mass stars.
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