Western Veil Nebula
The Western Veil Nebula is a supernova remnant consisting of oxygen, sulfur, and hydrogen gas. This area of Cygnus is densely populated with stars and includes regions of heated gas that make up the Cygnus Loop.
As APOD so eloquently puts it, the Western Veil Nebula is “an expanding cloud born of the death explosion of a massive star”. NGC 6960 (Caldwell 34) is often referred to as the Witch’s Broom as its delicate filamentary structure resembles this memorable shape.
On this page, you will see astrophotography image examples using a DSLR camera, and a one-shot-color astronomy camera using narrowband filters. My latest edition of the Western Veil Nebula was captured from my Bortle Class 8 skies in Ontario, Canada.
The Witches Broom Nebula (Western Veil) through a 102mm telescope
The image above was captured using a one-shot-color astrophotography camera through a small refractor telescope. A duo-narrowband filter was used to help isolate the light wavelengths associated with hydrogen and oxygen gases (Ha and OIII). You can view a larger version of this image on Flickr.
Learn more about the filters I use for astrophotography: Light Pollution Filters for Astrophotography
Video: Photographing the Veil Nebula
The video below takes you through the process of photographing the Veil Nebula, specifically the Western Veil Nebula and Pickering’s Triangle. I used a 430mm refractor telescope (William Optics Zenithstar 73) to capture most of the Cygnus Loop, leaving out the Eastern Veil Nebula.
To capture this image, a quad-band filter was used to isolate the prominent gases in the nebula. The OPT Triad Ultra filter (2″) was threaded to the field flattener of my telescope and sits in front of the camera sensor.
The video above features the first time I was able to capture Pickering’s Triangle as well as the Western Veil Nebula in a single frame. The resulting image below should give you a good idea of how wide this area of the sky is (over three times the size of the full Moon!)
The Witch’s Broom and Pickering’s Triangle captured using a DSLR Camera and Telescope.
The Western Veil Nebula
To capture the Veil Nebula through astrophotography requires patience, and a specific image processing approach. NGC 6960 resides in a countless sea of stars that must be tamed before the Western Veil Nebula will emerge.
Below, is a wide field photo of the Western Veil Nebula captured using a DSLR camera and a small refractor telescope. A DSLR camera like the Canon EOS Rebel Xsi used for the shot below is a great way to enjoy deep sky astrophotography through a telescope.
The camera had recently been modded for astrophotography by manually removing the stock IR cut filter above the sensor. This modification certainly helps to record more structure in nebulae such as this, but it is not essential to photograph the Veil Nebula.
NGC 6960 – Western Veil Nebula (DSLR)
Photographed on: July 8, 2014
Telescope: Explore Scientific ED80 with WO Flat III 0.8x FR/FF
Mount: Skywatcher HEQ-5 Pro
Guiding: Meade DSI Pro II and PHD Guiding
Guide Scope: Orion Mini 50mm
Camera: Canon EOS 450D (Modified)
Total Exposure: 4 Hours (60 x 240 seconds)
Processing Software: DeepSkyStacker, Photoshop CC
Support Files: 15 dark frames
Using Narrowband Filters
In August of 2017, I attempted to capture the Western Veil Nebula using Narrowband images from a color camera, the Altair Hypercam 183C. The image below adds Ha and OIII details to the true color broadband data for a Narrowband/RGB Composite.
The RGB details of this image were captured using a UHC filter (Ultra High Contrast). The Baader UHC-S was effective at reducing much of the unwanted light from my backyard sky, although I prefer the more natural look the Baader Moon and Skyglow (Neodymium) filter creates.
Altair Hypercam 183C (Narrowband)
Telescope: Explore Scientific ED102 CF
Camera: Altair Hypercam 183C
Mount: Sky-Watcher HEQ5 Pro SynScan
Guide Scope: Altair Starwave 50mm
Guide Camera: Altair GPCAM2 AR0130 Mono
Software: Astro Photography Tool, DeepSkyStacker, Adobe Photoshop CC 2017
Filters: Baader UHC-S, Astronomik 12nm Ha, OIII
Dates: July 29, Aug. 5, 8, 9, 14, 16
Ha: 47 x 300″ Bin 2×2
OIII: 64 x 180″ Bin 2×2
Baader UHC-S: 13 x 180″ Bin 2×2, 29 x 120″ Bin 2×2
Total Exposure: 8 Hours, 17 Minutes
Observing the Western Veil Nebula
This supernova remnant is believed to be produced over 5000 years ago. The Cygnus Loop contains the Eastern Veil Nebula and additional emission nebulosity of the same composition. This is one of my favorite nebulas to observe visually. Under the right conditions, you can follow the tendrils from end to end.
A telescope with a large aperture is needed, and an OIII filter will help. The Western Veil Nebula contains a naked-eye star known as 52 Cygni, which will help you locate the nebula with your telescope.
Below, you will see my photo of the Eastern Veil Nebula nearby. The focal length of my telescope (roughly 600mm) could not fit both objects in the same field of view.
This image of the Western Veil Nebula was photographed from a friends house out in the country with darker skies than I am used to from the backyard. The toughest part about processing this image of the Western Veil Nebula was reducing the brightness of the stars that surround the nebula. NGC 6960 is located in a very dense area of the Cygnus constellation.
Because the surface brightness of the Veil is relatively low, you must stretch the data in the nebulosity to create the contrast between it and the starry background. I use the “make stars smaller” action found in Noel Carboni’s Astronomy Tools Action Set, and ran the image through multiple iterations of this command.
It is helpful to mask the nebula while performing this action so you do not lose detail in the object itself.
Deep Sky Nebulae in Cygnus for Astrophotography
Here are some more excellent deep sky astrophotography targets in the constellation Cygnus that I have captured over the years.
- NGC 7000: The North America Nebula
- NGC 6992: The Eastern Veil Nebula
- NGC 6888: The Crescent Nebula
- IC 5070: The Pelican Nebula