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IC_1340, Stephen Duffy

IC_1340

IC_1340, Stephen Duffy

IC_1340

Description

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,a supernova remnant, many portions of which have acquired their own individual names and catalogue identifiers. This is a portion of the Eastern Veil (also known as Caldwell 33), whose brightest area is NGC 6992, trailing off farther south into NGC 6995 (AKA IC 1340 and the Bat nebula,shown). Some parts of the nebula appear to be rope-like filaments. The standard explanation is that the shock waves are so thin that the shell is visible only when viewed exactly edge-on, giving the shell the appearance of a filament. At the estimated distance of 2400 light-years, NGC 6995 spans only 1/2 degree, about the apparent size of the Moon. That translates to 12 light-years at the Veil's estimated distance. Undulations in the surface of the shell lead to multiple filamentary images, which appear to be intertwined. Text from Wikipedia

Mount: Paramount MYT
Scope: Vixen VCL200 @ F6 1278mm F/L
Camera: QSI 683

R:G:B 2h:2h:2h binned 2x2
For this image I wasted a lot of time taking luminance, Ha, and O3 frames that I ended up not using. The RGB looked the best.

Taken from Mendocino NF, July 2022
Reprocessed Dec 2022

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Histogram

IC_1340, Stephen Duffy