Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  IC 1871  ·  LBN 672  ·  LBN 673  ·  LDN  ·  Sh2-199
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Inside the Soul Nebula, James R Potts
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Inside the Soul Nebula

Getting plate-solving status, please wait...
Inside the Soul Nebula, James R Potts
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Inside the Soul Nebula

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Description

I saw one person on Astrobin who referred to this as "the Fire inside the Soul,"  I like that description.  And I am not complaining, as I'm really happy with this image and I didn't spend 2 days editing, changing, & deleting.  It came together pretty quickly.  The only thing I debated over was how much noise to reduce, I went with less, as I love the wispy details in the nebula, especially when you zoom in on the image.  There is some noise at the top of the image, I guess I could have tried to use the blur tool, but overall I think this turned out nicely and I hope everyone else thinks so, but as always, if you have suggestions or critiques, they are very welcome.  

This is only about 4.5 hours of data captured over 3 nights, in between clouds and other targets.  I actually made a mistake last night in my Auto Capture in the ASIAir pro, which I think helped this image.  I was going to capture 20 Ha, 10 Su & 10 OIII.  But I ended capturing 20 Su and no OIII.  When reviewing the individual FIT files, there is much more sulfur emissions that show up in this target than OIII (very little OIII).   I used the SHO 2 formula (Hubble Palette) in APP to combine images taken with Ha, Su & OIII fitlers.  In PS, I used Star Terminator to remove the stars and then I used an HSO combined image to add the stars back as a Luminance layer, which produced much better star color.

The dark  dust clouds outlined by bright ridges of glowing gas are cataloged as IC 1871. About 25 light-years across, this field of view spans only a small part of the much larger Heart and Soul nebulae. At an estimated distance of 6,500 light-years the star-forming complex lies within the Perseus spiral arm of the Milky Way.  The dense star-forming clouds of IC 1871 are a result of intense winds and radiation of the region's massive young stars.

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