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Sh2-190 Emission-Line Image, Alex Woronow

Sh2-190 Emission-Line Image

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Sh2-190 Emission-Line Image, Alex Woronow

Sh2-190 Emission-Line Image

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Description

Sh2-190 in True-Color SHO Extracted Emission Lines

OTA: Star-Fire 175 (f/8)
Camera: FLI - PL16070AE
Observatory: Deep Sky West. NM

EXPOSURES:
R: 12 x 600        
B: 15 x 600    
G: 13 x 600    
H: 21 x 1800
S: 21 x 1800
O: 16 x 1800

Total exposure: 35.3 hours
Image Width: 1.4 deg
Processed by Alex Woronow (2022) using PixInsight, Topaz, and PI-Scripts of my making

The image colors are “true colors” mapped from the colors of the extracted emission lines. Star colors are photometrically calibrated and transferred from an RGB image. The image displays an SHO emission-line-only image with the continuum emissions removed. In addition to providing the stars, the RGB images allowed computing the emission-line-only fluxes. The main image is a starless version. If you must see the stars, they appear in image B.

This nebula lies about 7500 lyr away. It is strongly shaped and stimulated into emission by a small group of stars near the center of an expansive “bubble.” Only a portion of that bubble appears in this image. The star cluster driving the bubble lies toward the top-center of the image.

Alex W

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  • Final
    Sh2-190 Emission-Line Image, Alex Woronow
    Original
  • Sh2-190 Emission-Line Image, Alex Woronow
    B

B

Title: Image with stars replaced

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Sh2-190 Emission-Line Image, Alex Woronow