IC1318 (Gamma Cygni area)
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About this Image
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The mag 2 star Gamma-Cygni or Sadr in the center of this image lies in the center of the Swan constellation, embedded in emission nebulae.
The distance to this area is estimated at approx. 1600 light years.
The nebula, which extends well beyond the borders of this image, is excited by young, hot blue-white stars and separated by dark nebulae into at least five major parts. The brightest of these parts is IC 1318,
The bisected nebula region east (right) of Gamma Cygni which is named the Butterfly Nebula because of its two-winged appearance.
The open star cluster NGC 6910 is situated half a degree north (below) and slightly east of gamma-Cygni. This group consists of 66 stars of 10th magnitude and fainter.
North is down.
Below you see a pure H-alpha monochrome image.
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Clic here for 60% size 2388x1590 (1037 kB)
Technical Details
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Optics |
105mm TMB refractor with flattener at f/6.5
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Mount |
MK-100 GEM |
Camera |
SBIG STL-11000M at -20C, internal filter wheel |
Filters |
Astronomik H-alpha (15 nm) + RGB |
Date |
H-alpha: May 11, 2004.
RGB: June 14, 2004 |
Location |
Wildon/Austria |
Sky Conditions |
mag 5.5, high transparency, temperature 10-15 C, before dawn |
Exposure |
Ha = 100 minutes (10-minute sub-exposures), RGB= 15:15:15 min (5-minute sub-exposures)
all 1x1. |
Processing |
Image aquisition in Maxim DL 4.0; Image calibration, aligning, mean stacking, DDP and color synthesis in ImagesPlus; Noise reduction by Neatimage; Photoshop: H-alpha blended to red and L channel; size 19/35/60%; |