Simon Addis
NGC6888 Crescent Nebula
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. It was discovered by Friedrich Wilhelm Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 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. (Wikipedia)
Narrowband image: 29/4 & 11/5/15
Oxfordshire, UK
4 Hours Total Exposure
Bin 1x1: 6x1200s Ha
Bin 2x2: 7x600s SII, 5x600s OIII
Equipment:
T: Takahashi FSQ106ED
C: QSI683ws Mono CCD, Astronomik Filters (6nm Ha)
M: Celestron Advanced Vx
G: QHY5-II
Acquisition and Processing:
PHD2, Sequence Generator Pro, CCDStack2, Photoshop CS6
NGC6888 Crescent Nebula
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. It was discovered by Friedrich Wilhelm Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 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. (Wikipedia)
Narrowband image: 29/4 & 11/5/15
Oxfordshire, UK
4 Hours Total Exposure
Bin 1x1: 6x1200s Ha
Bin 2x2: 7x600s SII, 5x600s OIII
Equipment:
T: Takahashi FSQ106ED
C: QSI683ws Mono CCD, Astronomik Filters (6nm Ha)
M: Celestron Advanced Vx
G: QHY5-II
Acquisition and Processing:
PHD2, Sequence Generator Pro, CCDStack2, Photoshop CS6