Observation by Peter Goodhew FRAS: Strottner-Drechsler Object 30

Uploaded by

Peter Goodhew FRAS

Observer

Peter Goodhew FRAS

Observed

2022 Jan 31 - 18:41

Uploaded

2022 Mar 24 - 19:01

Planetarium overlay









Constellation

Eridanus

Field centre

RA: 05h06m
Dec: -10°47'
Position angle: -10°17'

Field size

0°37' × 0°25'

Equipment
  • APM TMB LZOS 152 Refractors
  • QSI6120 CCD Cameras
  • 10Micron GM2000 HPS mount
Exposure

53 hours 25 minutes image capture (HaOIIISIIRGB)

Location

Fregenal de la Sierra, Spain

Target name

Strottner-Drechsler Object 30

Title

Strottner-Drechsler Object 30

About this image

A particularly interesting and at the same time enigmatic cosmic object.
In 2020, our team discovered "Strottner-Drechsler Object 30" in the constellation Eridanus - the nature of which is still unknown.
Despite the creation of a spectrum, it could not be clarified what exactly this nebula is.
Particularly exciting about Strottner-Drechsler Object 30 are the striking arcs and rings that could be detected in various chemical elements.
The core of the structure also shines particularly brightly in the ultraviolet spectrum.
However, we could not find a hot star responsible for the shape.
The photo shows the nebula in false colours with ionised hydrogen (H-alpha) coloured in blue and ionised sulphur (SII) in red.
Oxygen (OIII) could not be detected despite a very long exposure time.
Coordinates: 05:06:19.83 -10:47:37.37
Diameter: 7 to 10 arc minutes
Image captured on my remote dual rig at Fregenal de la Sierra in Spain between 19-31 January 2022.
Image processed by my dear friend Marcel Drechsler
More information at https://www.imagingdeepspace.com/stdr-object-30.html

Files associated with this observation
Like this image
Copyright of all images and other observations submitted to the BAA remains with the owner of the work. Reproduction of work by third parties is expressly forbidden without the consent of the copyright holder. By submitting images to this online gallery, you grant the BAA permission to reproduce them in any of our publications.