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

Eastern Veil NGC6992

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

Eastern Veil NGC6992

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


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