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M16: Emission Lines (SHO) Separated from the Continuum, Alex Woronow
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M16: Emission Lines (SHO) Separated from the Continuum

Getting plate-solving status, please wait...
M16: Emission Lines (SHO) Separated from the Continuum, Alex Woronow
Powered byPixInsight

M16: Emission Lines (SHO) Separated from the Continuum

Equipment

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Description

M16: Emission Lines (SHO) Separated from the Continuum

OTA: 10” home-made Newtonian, f/5.3
Camera: ASI 1600MM
Observatory: BlackRig

Exposures:
R:  13 x 600 sec
G:  18 x 600
B:  15 x 600
H:  11 x 600 sec
O: 15  x 600
S:  10 x 600
Total Exposure time used: 13.7 hours
Image Width: 45 arc minutes

Processing: PixInsight, Topaz Studio2 Luminar Neo, Aurora HDR, custom scripts for image weighting and star replacement

A big thanks to the altruism of BlackRig for providing these data absolutely free!

The image presented here has had the actual emission line radiation (i.e., photon contribution) separated from the spectral continuum. The continuum adds photons at all wavelengths, diminishing the contrast at feature boundaries and "blur" the color spatial locations across the image. Isolating the locations of the emission lines increases the delineation of features. At the same time, reflection nebulae are suppressed… c'est la guerre!
(However, in this case, I did not have information about the narrow band filters' bandwidth, so some reflection nebulae probably crept through.)

Compute with power!

Alex Woronow

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M16: Emission Lines (SHO) Separated from the Continuum, Alex Woronow