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Soul Nebula Closeup, Part of LBN 673 and W 5

 

MOUSE-OVER IMAGE FOR STARLESS VIEW

MOUSE-OVER IMAGE FOR STARLESS VIEW

CLICK ON IMAGE FOR FULL SIZE VIEW (4817x7608)

 

Scope: Celestron 9.25 Edge HD 235 mm at f/7;  

Location: DAA Observatory, Shelter Valley, CA;  

Dates: 2, 26, 27 August, 2024;  

Camera: ASI294MM (Baader  Ha, OIII, RGB Filters);

Exposure:  16.5 hrs

RGB - 32 x 1.5 min (gain-121 2x2) each RGB exposures.,

Ha - 124 x 3.5 min (gain-160 2x2,

OIII - 118 x 3.5 min (gain-160 2x2),

 

Processing: 

Data Collection -  N.I.N.A. Sequencer (as FITs).  Sub-frame calibration - Pixinsight (WBPP). 

Sub-frame  registration and integration (Average combine -  Linear clipping) - PixInsight (WBPP).  

Noise reduction - NoiseXTerminator - PixInsight. 

Non-linear stretching, normalization and gradient removal - PixInsight.

Photometric RGB calibration (SPCC) - PixInsight. 

Deconvolution of  Lum, Ha, OIII, and RGB stacks (RGB combine) - BlurXTerminator. 

Generation of starless nebulosity Lum, Ha, OIII , and RGB images for later processing - StarXTerminator.  

Curves, Levels, RGB combine - PixInsight.  RGB Stars and starless  combine - PixInsight.   

Final finishing  - Affinity Photo.   

Annotation - PixInsight, Aladin (Simbad ), and Affinity Photo. 

This image is a  modified HOO Narrow Band  and screened RGB starless construction - with RGB stars added.  Image processed at 6248x4176 resolution. 

Final Image size is approximately  4817x7608.

 

Description:

North is left in this image.  This image is a close-up of an interesting region within the Soul Nebula, IC 1848. It evokes the idea of a small man climbing a mountain to reach the stars.

Aside from this climbing imagery the universe is showing us, the image has some dark nebulae within. TGU H879 P16, Dobashi 3918, and Dobashi 3919 are the dark nebula toward the center of the image. 

The bright nebula around Dobashi 3913 (center of the image) is an ISM structure RNO 11 - sometimes referred to by the name 'LW Cas Nebula'. The top of the image is the northern half of LBN 673 - a north/south band of hydrogen emission.

IC 1848 is known as a star forming region. A study in IR wavelengths produced a catalog of star forming in the Westerhout 5 / IC1848 region - [KAG2008] (Koenig, Allen, Gutermuth et al.). Over 17,000 sources were identified. About 900 were deemed 'extragalactic' and thus eliminated. 18 were identified as 'Globules'. This image contains three of those Globules - Globule 10, 11, and 13. Globule 10 and 11 are 'trunk' types - the 'mountain' peaks  above the little man; 13 is a cometary type globule toward the bottom of the image.

 

These objects and some of the brighter stars are identified in the annotated image Vertical FOV is approximately 0.61 degrees. Full size image scale is about 0.29 arcsec/pix.

Image center is approximately - 

Equatorial 2000: RA: 06h 46m 52s Dec: +06°24'47"

 

 

All images and content remain the property of Jim Thommes - copyright 2003 - 2025

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