Gamma Cygni Nebula and NGC6888 (Crescent Nebula)

IC1318
All Images Copyright Steve Cannistra

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Characteristics:
RA (J2000): 20h 19m 32s
Dec (J2000): +39 degrees 35' 08"

Description:
The Gamma Cygni Nebula is an expansive emission region in the constellation Cygnus, shown here as an HOO image using a dual HaOIII filter (more details below).  The star Sadr (aka Gamma Cygni) is the brightest in this field of view, seen in the right lower quadrant of this image, and is actually not part of the nebula itself, being in the foreground and located approximately 1,800 light years away. In contrast, the IC1318 nebula is more distant at 5,000 light years away and emits Ha and OIII light as a result of being ionized by intense UV irradiation from many highly luminous Cygnus OB2 association stars embedded within the nebula.  These stars are not easily observed in this image due to the obscuring effects of intervening dust throughout this region.  The entire nebula is a stellar nursery in which stars are being formed as a result of gravitational collapse of surrounding hydrogen gas (and other heavier elements such as helium and oxygen).  Also seen in this image is the Crescent Nebula (NGC6888)
in the left upper quadrant, an emission nebula excited by intense UV irradiation from its central star, WR136.  Wolf-Rayet 136 has shed its outer, hydrogen layers and is burning helium in its core, and is expected to have a lifespan of only several million years (compared to our Sun, which is a lower mass G2V star with an expected lifespan of 10 billion years).  I previously imaged the Crescent Nebula at a longer focal length and also obtained the spectrum of WR136, shown here.  More information about this interesting region can be seen on Rob Gendler's Website .

Photographic Details:
Dates:  June 1 and 3, 2026.
Scope:  SV555 243mm lens (54mm aperture at f4.5) on the ZWO AM3N mount.  This is my new, portable set up.
Autoguider:  ASI178 autoguider with SvBony 30mm guidescope, focal length 120mm.
Camera:  ZWO ASI2600MC at 0C; Pixel size 3.76 microns (Bin 1x1), yielding an image scale with the SV555 (243mm focal length) of 3.19 "/pixel.
Filter:  SvBony HaOIII 7nm Dual Narrowband filter .
Image acquisition software:  ASIAIR Plus (necessary for me now, since I need a completely portable imaging rig that allows me to travel to a nearby imaging site).
Exposures:  Total exposure 8 hours, 300 second subs.
Processing:  Calibration and integration in Pixinsight.  Separation of image into Ha and OIII components using DBXtract.  Assembly of HOO image in Pixinsight, followed by separation of stars/nebula components using StarXTerminator.  Deconvolution (BlurXTerminator), and noise reduction (NoiseXTerminator) in Pixinsight.  Subsequent processing in Photoshop.

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