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NGC2403 in Camelopardalis
Enhanced Hydrogen Comparison
Spiral
galaxy in Camel
Uploaded
1/1/07
This comparison illustrates
that when the large amount of hydrogen present in this galaxy
is made more easily visible, the entire galaxy became swamped
with the pink light of swirling hydrogen clouds. Once again,
you will easily be able to see that many of the blue stellar
OB associations present in the arms are intimately connected
with thier accompanying hydrogen regions. The right side of this
spiral is so intense with gas, that the entire appearance of
the galaxies arm is changed.
This years rendition
of this splendid face on spiral in Camelepodarus incorporates
the latest processing techniques, and plenty more color data
for a rich and very low noise presentation. NGC2403 is a low
surface brightness inclined Sc spiral, rated at an integrated
magnitude of 8.9, which is spread out to a rather thin 25 arcseconds
in size - about half a degree long here. North is up in this
view, and the galaxy is inclined about 5 degrees from face on
for our view from the Earth. Additionally, this galaxy is very
dust obscured, with a B-V index of.47, meaning it photographs
as nearly pure yellow. Histogram equalization was able to easily
correct for this discoloration, presenting the galaxy in a more
true color appearance.
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Instrument: 12.5" f/5 Home made Newtonian
Mount: Astrophysics 1200 QMD
CCD Camera: SBIG 10XME NABG with Enhanced Water Cooling
Guider: SBIG ST4 w/Lumicon Newt Easy Guider
Exposure: LRGB = 80:40:40:40 (RGB Binned 2x2)
Enhanced Image add 2h of Ha data
AstroDon RGB Combine Ratio: 1: 1.05: 1.11
Location: Payson, Arizona, Elevation: 5150 ft.
Sky: Seeing FWHM = 4.5 arcsec (Maxim DL - 10min subframe), Transparency 8/10
Outside Temperature: 35 F
CCD Temperature: -30 C
Image Processing Tools:
Maxim DL: Calibration, Deblooming (Starizona Debloomer), aligning, stacking
Gralak's Sigma: Stacking
PixInsight: Curves, Deconvolution, noise reduction
Photoshop CS2: Curves, Color Correction, Gradient removal (Grad Xterminator), Cleanup
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