Emission nebula in constellation Cygnus.
Sh2-114 is a weak emission nebula in the constellation cygnus and has a slightly torn shape. The area obviously consists of several arcuate filaments lying on top of each other.
Object: | Sh2-114 |
Date of exposures: | 03.09.2018, 04.09.2018, 05.09.2018, 15.09.2018, 16.09.2018 |
Exposures: | Ha 5nm: 154 x 300", OIII 3nm: 59 x 300", RGB: 78 x 300", Sum: 24,3 hrs. |
Telescope: | 10'', F4 Newton |
Focal length: | 1000mm |
Filter: | Astrodon RGB E-Series, H-Alpha 5nm, OIII 3nm |
Camera: | ASI 1600 MMC Pro |
Guiding: | Off Axis Guider, Lodestar |
Mount: | EQ8 |
The arcs have a semicircular shape with a depression facing south. It is suspected that this, together with the nearby Sh2-113 cloud, is a bubble shape that looks like a supernova remnant. To date, however, no supernova has been recorded or described in this region.
At the upper edge of the image is Kronberger (Kn) 26 - a bipolar emission nebula. A detailed analysis of the morphology and kinematics indicates the possible presence of two pairs of bipolar wings that would make Kn 26 a new member in the four-pole PN class.
The image was taken in 5 nights with over 24 hours exposure time from Ha, OIII and RGB images. Here the whole field: