Hemisphere:  Northern  ·  Constellation: Auriga (Aur)  ·  Contains:  20 rho Aur  ·  Sh2-223  ·  Sh2-224  ·  The star ρAur
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Sh2-224 & Sh2-223, 



    
        

            Gary Imm
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Sh2-224 & Sh2-223

Getting plate-solving status, please wait...
Sh2-224 & Sh2-223, 



    
        

            Gary Imm
Powered byPixInsight

Sh2-224 & Sh2-223

Imaging telescopes or lenses: Takahashi FSQ-85ED

Imaging cameras: ZWO ASI 1600MM Cooled Pro

Mounts: Astro-Physics Mach1GTO

Guiding telescopes or lenses: Orion 60mm Guidescope

Guiding cameras: Orion StarShoot AutoGuider Pro Mono

Focal reducers: Takahashi Reducer QE 0.73X

Software: Main Sequence Software Sequence Generator Pro  ·  PixInsight  ·  Stark Labs PHD2 2.6.3

Filters: Astrodon Ha 31mm 5nm  ·  Astrodon OIII 31mm 3nm  ·  Astrodon Green 31mm Gen2 I-Series  ·  Astrodon Blue 31mm Gen2 I-Series  ·  Astrodon Red 31mm Gen2 I-Series

Accessory: ZWO EFW  ·  Feathertouch Focuser Boss II Electronic Focusing Control


Dates:Dec. 1, 2018Dec. 2, 2018Dec. 3, 2018

Frames:
Astrodon Blue 31mm Gen2 I-Series: 30x60" (30') (gain: 139.00) -20C bin 1x1
Astrodon Green 31mm Gen2 I-Series: 30x60" (30') (gain: 139.00) -20C bin 1x1
Astrodon Ha 31mm 5nm: 54x300" (4h 30') (gain: 300.00) -20C bin 1x1
Astrodon OIII 31mm 3nm: 54x300" (4h 30') (gain: 300.00) -20C bin 1x1
Astrodon Red 31mm Gen2 I-Series: 30x60" (30') (gain: 139.00) -20C bin 1x1

Integration: 10h 30'

Avg. Moon age: 24.75 days

Avg. Moon phase: 24.15%


Astrometry.net job: 2408714

RA center: 5h 22' 0"

DEC center: +42° 19' 33"

Pixel scale: 2.383 arcsec/pixel

Orientation: -36.248 degrees

Field radius: 1.826 degrees


Resolution: 4526x3160

Locations: Backyard (Mag 20.8 - Bortle 4.5), Onalaska, Texas, United States

Data source: Backyard

Description

This image captures two very faint and fascinating objects, Sh2-224 to the left and Sh2-223 to the right, located in the constellation of Auriga. It is amazing to me that these two rare objects can be captured in the same field of view. Both of these objects have been classified as supernova remnants (SNRs), which they appear to resemble optically. But these two objects are no longer believed to both be SNRs.

Sh2-224, located 12,000 light years away, has plenty of Ha and OIII signal, characteristic of all SNR that I have imaged. The primary section on the left side is spherical with an apparent diameter equal to our full moon. The much wider wing just to the right occurred from an eruption of the spherical SNR into a very low density cavity of the interstellar medium. Once erupted, the SNR rapidly expanded into the low density cavity, creating the larger wing. I don't quite understand everything about how this mechanism works, but the result is visually very interesting. We are fortunate to have this perspective from earth's view - views from other perspectives would make it difficult to understand the mechanism. My mind tends to think that empty interstellar space is uniform, but obviously it is not empty nor uniform. The SNR is believed to be 60,000 years old and currently spans 150 light years. It is believed to be one of the older SNRs. The progenitor star for this SNR has not been identified.

Although Sh2-224 is huge, Sh2-223 is even larger. It has been identified in numerous sources as one of the largest SNRs known. I was surprised that I found no oxygen in the nebula, unlike all of the other SNRs I have imaged. After further digging, I discovered that a paper published in 2006 (The Galactic H II region OA 184 by Foster/Kothes/Sun/Reich/Han) has concluded that this object is not a SNR as many sources describe. Instead, it is a HII region energized by the lone star BD+41 1144 (identified in the attached annotated image). The paper also gives this object a new distance of 7000 light years. The spherical, SNR-like shape of this HII region is unlike that of any HII region that I can recall imaging.

Despite its demotion from SNR status, SH2-223 is still a big beautiful object as it hangs alongside its SNR neighbor Sh2-224 in the bright, colorful star-filled sky of Auriga.

Comments

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    Sh2-224 & Sh2-223, 



    
        

            Gary Imm
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  • Sh2-224 & Sh2-223, 



    
        

            Gary Imm
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Sh2-224 & Sh2-223, 



    
        

            Gary Imm