Hemisphere:  Southern  ·  Constellation: Sculptor (Scl)  ·  Contains:  NGC 131  ·  NGC 134
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NGC 134, 



    
        

            Gary Imm
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NGC 134

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NGC 134, 



    
        

            Gary Imm
Powered byPixInsight

NGC 134

Imaging telescopes or lenses: Takahashi TOA-130NFB

Imaging cameras: ZWO ASI 183MM Pro Cool

Mounts: Astro-Physics Mach1GTO

Guiding telescopes or lenses: Orion 60mm Guidescope

Guiding cameras: Orion StarShoot AutoGuider Pro Mono

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

Filters: Astrodon Green 31mm Gen2 I-Series  ·  Astrodon Blue 31mm Gen2 I-Series  ·  Astrodon Lum 31mm Gen2 I-Series  ·  Astrodon Red 31mm Gen2 I-Series

Accessory: Feathertouch Focuser Boss II Electronic Focusing Control  ·  ZWO EFW  ·  Takahashi Flattener TOA-67


Dates:Aug. 29, 2019

Frames:
Astrodon Blue 31mm Gen2 I-Series: 30x120" (1h) (gain: 111.00) -12C bin 1x1
Astrodon Green 31mm Gen2 I-Series: 30x120" (1h) (gain: 111.00) -12C bin 1x1
Astrodon Lum 31mm Gen2 I-Series: 60x120" (2h) (gain: 111.00) -12C bin 1x1
Astrodon Red 31mm Gen2 I-Series: 30x120" (1h) (gain: 111.00) -12C bin 1x1

Integration: 5h

Avg. Moon age: 28.44 days

Avg. Moon phase: 1.34%


RA center: 00h30m21s.900

DEC center: -33°1434.15

Pixel scale: 0.494 arcsec/pixel

Orientation: 179.286 degrees

Field radius: 0.335 degrees

More info:Open 


Resolution: 3996x2808

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

Data source: Backyard

Description

This object is a barred spiral galaxy located 60 million light years away in the constellation of Sculptor at a declination of -33 degrees. The galaxy spans 9 arc-minutes in our apparent view, which corresponds to a diameter of 100,000 light years.

Our view of the galaxy structure is hindered by its 78 degree inclination angle, which is a shame because the structure looks very interesting. This is designated as a barred galaxy although is is difficult for me to see that here. An S-shaped yellowish inner disk region, including a bright core, contrasts with the blue diffuse outer arms. At the convergence between the two, faintly reddish areas indicate possible HII regions. The dark lanes are detailed and appear to be broken up throughout the disk. Sources indicate that the galaxy disk is warped. It is apparent to me that the disk is a bit distorted, but it doesn't look warped to me in this image.

The small galaxy at left is NGC 131. Distance estimates of it vary. Some estimates put it about the same distance away as NGC 134, which could be the cause of the disk distortion. Another possible culprit is the low surface brightness galaxy on the right, ESO 350-26.

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