Eastern Veil - NGC6992 in Cygnus
The Veil Nebula, is part of the Cygnus Loop, radio source W78, or Sharpless 103. Other parts of the loop include the 'Eastern Veil', the 'Western Veil' or 'Witch's Broom Nebula', and Pickering's Triangular Wisp. It is a large, relatively faint supernova remnant in the constellation Cygnus. The source supernova exploded some 5,000 to 8,000 years ago, and the remnants have since expanded to cover an area of ~3x3 degrees; about 6 times the diameter or 36 times the area of a full moon. The distance to the nebula is not precisely known, with estimates ranging from 1,400 to 2,600 light-years. It was discovered on 1784 September 5 by William Herschel.
Picture presents its eastern part.
Western part can be found HERE .
Entire Veil SNR can be found HERE
Photo Details
Telescope: Sky90 at f4.5 Takahashi
Camera: Asi1600MMC-p
Mount: HEQ5 belt moded
Guiding: Off-axis Lodestar
Exposure: H 7x10min, O3 10x0min, RGB 4x2min each Unity Gain
When: August 2019
Other information: final test vefore BBB2019 trip
Photo Details
Telescope: FSQ106EDX (530 mm) Takahashi
Camera: Sbig ST-8300M Filter wheel, Baader 36mm HLRGB filters
Mount: NJP Takahashi
Guiding: Off-axis SS Orion
Exposure: Ha 20x20min RGB 6x8min each
When: July/August 2013
Other information: very good transparency, very good seeing 
Photo Details
Telescope: FSQ106EDX (530 mm) Takahashi
Camera: Sbig ST-2000XM, Filter wheel, Baader 1.25" HLRGB filtes, color taken with ST-2000XCM
Mount: NJP Takahashi
Guiding: Self-guided
Exposure: Ha 2.5h LRGB 2.5h
When: ----
Other information: good transparency, good seeing