This image contains the Crescent Nebula NGC 6888 near the left edge and surrounding nebulosity belonging to the γ Cygni Nebula Region.

Although it does look like a miniature version of the well-known Veil Nebula, NGC 6888 is in fact neither a supernova remnant nor a planetary nebula, but one of the rare Wolf-Rayet nebulae. As the name already suggests, at the heart of this nebula is a Wolf-Rayet star (the bright star located centrally within the nebula). These stars rank among the most massive and hottest stars known. Characteristic for Wolf-Rayet Stars are their strong stellar winds, approximately 2.000 kilometers per second, and the enormous mass-loss associated with them, they can lose an entire solar mass in only 10.000 years. The central star exhibits an absolute absolute magnitude of -4.4 mag, radiating thus 5.000 times more brightly as our sun, however the maximum energy output lies in the UV range.

The nebula is illuminated by two independent ionization procedures. One illumination source is the central star, which ionizes the nebula (particularly the [OIII] line) due to its strong UV emission. The other ionization source is the collision of the fast stellar winds with slower moving stellar winds from the earlier red-giant stage of the same star, which results in an impact front, which in turn heats up the material.

Wolf-Rayet stars and their nebulae are short-lived phenomena (in astronomical timescales), these stars will erupt in supernovae during the next million years.

The surrounding area contains several patches of emission nebulosity. The brightest parts are LBN 208 (upper left, filamentary structure), LBN 193 (lower left) und LBN 192 (lower right) in Lynd's Bright Nebulae catalog.

LBN 242 and Surrounding Nebulosity, Western Cygnus, telelens photograph.
NGC 6888 - Crescent Nebula, Wide Field in Hα, which is part of this image.
NGC 6888 - Crescent Nebula, Newtonian image.