Soul Nebula

Soul Nebula
IC 1848
9/20-26/2017
Cassiopeia
BrewSky Observatory, Casa Grande, AZ
Takahashi FSQ106ED on Paramount MX using SBig STF8300M camera with Bader filters
−5°C
# Exp (min) Filter Bin Net Time (hr)
18 1800 HAlpha 1×1 9
19 1800 OIII 2×2 9.5
16 1800 SII 2×2 8
29 1 (for stars) Red 1×1 .5
21 1 Green 1×1 .5
25 1 Blue 1×1 .5
Total 28 hr
Calibrated in MaximDL
Processed in PixInsight  (First use of ColorMask tool to get gold/blue look)SHO color palette, some mixing of channels
From Wikipedia:

Westerhout 5 (Sharpless 2-199, LBN 667, Soul Nebula) is an emission nebula located in Cassiopeia. Several small open clusters are embedded in the nebula: CR 34, 632, and 634 (in the head) and IC 1848 (in the body). The object is more commonly called by the cluster designation IC 1848.

Small emission nebula IC 1871 is present just left of the top of the head, and small emission nebulae 670 and 669 are just below the lower back area.

This complex is the eastern neighbor of IC1805 (Heart Nebula) and the two are often mentioned together as the “Heart and Soul”.

W5, a radio source within the nebula, spans an area of sky equivalent to four full moons and is about 6,500 light-years away in the constellation Cassiopeia. Like other massive star-forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region’s most massive stars. According to the theory of triggered star formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. The image in the gallery above contains some of the best evidence yet for the triggered star formation theory. Scientists analyzing the photo have been able to show that the ages of the stars become progressively and systematically younger with distance from the center of the cavities.