Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  IC 1340  ·  NGC 6995  ·  Network nebula  ·  Veil nebula
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Sharpless 2-103, a portion of the Veil Nebula Complex, flyingairedale
Sharpless 2-103, a portion of the Veil Nebula Complex
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Sharpless 2-103, a portion of the Veil Nebula Complex

Getting plate-solving status, please wait...
Sharpless 2-103, a portion of the Veil Nebula Complex, flyingairedale
Sharpless 2-103, a portion of the Veil Nebula Complex
Powered byPixInsight

Sharpless 2-103, a portion of the Veil Nebula Complex

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Sharpless 2-103 is an emission nebula that is part of eastern arc of the veil nebula (NGC 6992), one of the largest and well known supernova remnants in the northern sky. I couldn't find much information on Sharpless 2-103 but the field of view seems to share the same neighborhood with NGC 6995, which, according to Bob King's article in Sky & Telescope, "Explore the Veil Nebula", is the bright arc of material at the south end of NGC 6992 that unfurls to the west.  The article also notes that the nebula continues to expand outward since the supernova that created it thousands of years ago. Photos taken with the Hubble Space Telescope in 1997 compared with those from 2015 show individual filaments on the move. 

What captures my interest most in this image are the clearly defined filaments formed by dense concentrations of glowing Oxygen III (blue/green) created by the shock wave long ago . By contrast, the ionized Hydrogen (red) in this region is more diffuse and less well defined.

This image was created by mapping HOO narrowband images to RGB in Pixinsight. The data was taken through an RH-305 astrograph and FLI 8300 series camera at Deep Sky West.

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Sharpless 2-103, a portion of the Veil Nebula Complex, flyingairedale