Veil Nebula

Veil Nebula
0

Veil Nebula

A supernova remanent in the Cygnus constellation. The shock wave forms a bobble of ionized gas around the remanent. The image is an LRGBNB composite, I use 4X600s OIII exposures to enhance 8x300s B and G filters and 4x600s Ha to enhance the 8x300s R filter. Finally, a Luminance enhance was applied using Ha and 9x150s L filters.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
Takahashi FSQ-106ED
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL16083
Location ..........................................................................................................................................................................................................................
Location
IC Astronomy Observatory, Spain
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Jun 2021
Filters ..........................................................................................................................................................................................................................
Filters
LRGBHaOIII
Processing ..........................................................................................................................................................................................................................
Processing
PixInsight
Credits ..........................................................................................................................................................................................................................
Credits
H,Ibarra-Medel
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