I wasn’t satisfied with the outcome of my star handling program so I rewrote it. The goal was to obtain an image that is as technically accurate as possible, while contains less artifacts and it is more appealing than the original.
I recorded with the Canon 1100D mod 21×150 sec, ISO 1600, with the lens Canon EF 200mm f2.8L II USM dialed to F/4, mounted on the HEQ5. The main feature is the red glow of the ionized hydrogen region around γ Cygni (the brightest star in the frame) with dramatic gaps caused by clouds of dark nebulae. The Crescent Nebula is also there. The object is also known as NGC 6888, Caldwell 27, Sharpless 105, and is a nebula blown by the Wolf-Rayet star WR 136 (HD 192163) expected to go supernova in the next 100k years.









