Location & Date	Backyard, Abbott Observatory- Long Island, NY,  June 2022
Telescope	TMB130SS  910mm F/7 APO, Moonlite focuser, Losmandy G11 Gemini Image scale 1.54 arcsec/pixel
Camera	SBIG ST-10XME Baader Ha OIII  5nm filters CCD temp -15°C
Exposures	Ha- 14 x 10m  OIII- 18 x 10m   Bin 1x1
Planning & Acquisition	Sequence Generator Pro
Processing	CCDStack -  Calibration, Debloom, Normalize, Alignment, Combine, Deconvolution Adobe PS -  Ha + OIII combine, Color adjustments, Detailing,  Noise reduction, JPEG conversion RC-Astro Star XTerminator Topaz Sharpen This a bi-color palette where Ha=red, OIII=blue and Ha+OIII mixed to provide a synthetic green.

Wikipedia-

  The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.

  It is a rather faint object located about 2 degrees SW of Sadr. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".

NGC 6888 position shown relative to our location (Sun) in the Milky Way Galaxy

Galatic Longitude: 75.6

Galatic Latitude: 2.4

Distance from Galatic Plane:283 ly above the galatic plane

Above image and info provided by Our Galaxy 3D Atlas application and used with permission by Otherwise