This image is a 2 panel mosaic comprising 28 hours of RGB exposures in 20 minute sub-frames. The images were acquired across 8 nights during November December 2018. Processing is exclusively with Pixinsight.
This is the processed result of 10 hours worth of 20 minute RGB sub-frames.
Published in Astronomy Now: December 2018
The constellation Auriga contains two bright areas of Ha emission; IC405 and IC410. The Baby-Q with the Moravian G3-16200 has a large enough field of view that I can fit both into the same picture.
This is seven 20 minute exposures through my Baader 3.5nM Ha filter. Processed in Pixinsight.
Back in January I took a couple of 1 hour exposures of Sh2-216 using my Ha filter. Nearly one year later, a spell of good weather over a weekend meant that I was able to add a few more and I now have 10 hours worth.
Sh2-216 has been calculated at a distance of 129 parsec (420 light years) by measuring the parallax of the central star which places it much closer than the Helix and Dumbbell nebulae at 219 & 379 parsec respectively.
It measures about 2 arc degrees on the sky and is very faint.
It’s been a while since I last visited this object, a dust cloud on the Andromeda / Cassiopeia border (http://littlebeck.org.uk/?p=1058 & http://littlebeck.org.uk/?p=948). This is the first time with a monochrome camera and RGB filters; previous attempts have been with the KAF8300 equipped QHY9C OSC camera.
The field with the G3-16200 is much larger and provides a better context for the object. Better data, and much improved processing skills have revealed a lot more of the surrounding faint clouds.
This is about 12 hours of RGB data acquired in 10 minute subframes. I’m not a fan of LRGB imaging and very rarely use luminance, preferring instead to spend longer capturing the colour data at bin 1×1. Processing is exclusively Pixinsight.
Displaying the monochrome Ha image in a local exhibition of pictures was a spur to getting to grips with the colour data I’ve acquired for this image. With the Ha & RGB data this now amounts to 51 hours in 10 & 20 minute sub-frames.
The image is reduced to 40% of full size for display here (click on the thumbnail).
This object is the remnant of a supernova explosion that occurred some 40,000 years ago and the shell has been expanding ever since. It now spans about 3 degrees on the sky, which at it’s estimated distance of 3000 light years is 157 light years in diameter.
This image was published in the June 2017 edition of Astronomy Now.
It’s been a while since I last posted here. Images are posted first to the Breckland Astronomical Society Facebook page which a more interactive medium for discussion.
I’ve been busy in the meantime gathering images of the supernova remnant Simeis 147. This is a huge object requiring a 4 pane mosaic to cover it. So far I’ve only completed the Ha image to my satisfaction.
In 1966 when George Abell compiled his catalog of planetary nebulae entry 85 in Cassiopeia was mis-classified. While it has some resemblance to a planetary nebula it is subsequently been found to be the remnants of a supernova explosion . However, unlike the Cygnus loop it’s emission is mainly in H-a with very little O-III.
I’m still collecting data for this object but this is a process of the first 12 hours of images shot through a Baader 3.5nm Ha filter.
There is an older, fainter supernova remnant in Cygnus and it lies just up from the double star Albireo. At about 30000 years old (Veil 7500 years) and further away 2500 ly (Veil 1500 ly) it is correspondingly fainter. The part I’ve imaged here has the designation Sh2-91.
I last took pictures of this object back in 2014 with my QHY9 colour camera and it wasn’t entirely prominent but by combining the old data with 4 hours shot through my new Baader 3.5nm Ha filter a more distinctive image is formed.
I’ve rejected some of the original frames that had some thin cloud and re-stacked, then registered the new Ha frames and combined using the Pixinsight NBRGBCombination script.