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2021, December 2021 Jason Matter 2021, December 2021 Jason Matter

Flying Bat Nebula and Squid Nebula

Image Description and Details :

I present you my last acquisition since the setup HAO_4. these are two nebulae including one (Ou4) discovered by my friend the French astrophotographer Nicolas Outters in June 2011. This is the Giant Squid (in blue/green in the image) which is a bipolar planetary nebula located about 2000 light-years from Earth surrounded by the Flying Bat Nebula (cataloged Sh2-129 in red), both are located in the direction of the cepheus constellation.
Technical details:
- Apo Takahashi FSQ 85 to F/D 5.3
- iOptron 60 cem ec mount
- Asi 2600 mm pro
- Astronomik filters 6nm
- 205x300s HA : 17 h 05 min
- 188x600s O3 : 31 h 20 min
-181x300s S2 : 15 h 05 min
- 3 x 30 x 60s RGB : 1 h 30 min
- Full integration: 49 h 55 min
- DOF: 33/101/25
- Date: October/november 2021
- Location: HAO Observatory, Oukaimeden, Morocco.

Copyright: K. Aziz

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2020 Monthly Winners, 2020 Jason Matter 2020 Monthly Winners, 2020 Jason Matter

A Flying Bat (Sh2-129)

A Flying Bat (Sh2-129) with a Squid (Ou4) Inside?

I have been wanting to try this deep sky object for two years. It is quit interesting two objects for the prices of one. In reality I only have a portion of Sh2-129, the Flying Bat Nebula, which is a huge region of hydrogen gas represented by the red color captured with the Hydrogen gas filter (Ha). Located in Cepheus approximately 2,300 light-years away, Sh2-129 is a faint emission nebula and has been known about since at least the 1950's as a neighbor to IC 1396, the Elephant Trunk Nebula. I must admit, even after looking at widefield images of the Sh2-129, I see no resemblance to a Flying Bat. The Squid on the other hand does resemble a squid with it tentacles rapped up. The Squid Nebula (Ou4) is a relatively new discovery from 2011 by French astro-imager Nicolas Outters. It consists doubly ionized oxygen which gives it the green-blue color in contrast to the hydrogen. It may seem odd that this was not found until 2011 but there is a really good reason, it is really dim. I was taking 5-minute subs and while there was some nebulosity in the Ha region, there was nothing in OIII, not even a hint. If you are the type that likes to complete an object in one night, then this would not be a good choice.

Originally the Ou4 was thought to be a Planetary Nebula unrelated to Sh2-129, however, recent studies suggest it is within Sh2-129 and is bipolar outflow from a triple star system. The bright blue star in the center is the believed to be the source.

I wanted to get at least 15-hours and was able to get this done quicker than I anticipated due to unexpected clear weather. It worked out really well as we had a succession of clear nights when I was painting my garage floor anyway so conveniently left everything set up and just put a cover over it. This was one of the hardest things I have processed due the conflicting things going on. The Ha data was really strong and came out very well with hardly any processing. Not surprisingly, the OIII was very difficult to bring out and a lot of time was spent on it. StarNet was used to make separate starless Ha and OIII images which were combined to make a starless HOO image. The last part of the process was merging the RGB stars with the HOO starless image. This turned out be more difficult as the method I normally use for combining RGB stars with narrowband images didn't work well with the starless image so I used alternative method in PS described by Trevor Jones.

Camera: ZWO ASI1600MM-Pro

Telescope: Astro-Tech AT115EDT 115mm Refractor Telescope

Focal Reducer: AstroTech Field Flatterner/Focal Reducer

Mount: Orion Atlas Pro

Filter Wheel: ZWO EFW 8 x 1.25"

Filter: ZWO Ha, OIII, R, G, B

Focuser: ZWO EAF

Autoguiding: ASI120 Mini attached to an Agena 50mm Guide Scope/ZWO 60mm Guidescope

Exposure: Ha 150 x 300s, OIII 165 x 300s, R 45 x 60s, G 29 x 60s, B 29 x 60s

Processing: APT, NINA, PixInsight, Photoshop.

Copyright: Kurt Zeppetello

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