description IRAS 20068+4051 Overview
IRAS 20068+4051 is a protoplanetary nebula in the constellation Cygnus, identified in infrared observations by the Infrared Astronomical Satellite, commonly abbreviated IRAS. It has a bipolar morphology, with material arranged in two opposing lobes, and an asymmetric envelope of dust. The object represents a short transitional stage in stellar evolution, after an aging star has expelled material but before the surrounding nebula reaches its later planetary-nebula form.
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