Veil Nebula

This image is a combination of LRGB frames and halpha and OIII mixed to the redchannel and the bluechannel

Image in HST-palette

Veilnebula LRGB

This is the “classic LRGB” version

The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus. It constitutes the visible portions of the Cygnus Loop (radio source W78, or Sharpless 103), a large but relatively faint supernova remnant. The source supernova exploded some 5,000 to 8,000 years ago, and the remnants have since expanded to cover an area roughly 3 degrees in diameter (about 6 times the diameter, or 36 times the area, of the full moon). The distance to the nebula is not precisely known, but recent evidence from the Far Ultraviolet Spectroscopic Explorer (FUSE) supports a distance of about 1,470 light-year

Optics/mount : 12″ACF 2.7m AP-Reduzer Alt-5
Camera/filters: Atik 11002 Astrodon LRGB halpha/OIII 5nm
Exposure: 5h LRGB 10min subs all 1xbin Ha/OIII 6h