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"WHEN
ROSES AREN'T RED" NGC
2244 - THE
ROSETTE NEBULA in "HUBBLE" COLORS Red = SII, Green
= Ha, Blue = OIII 2 frame MOSAIC
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About
this Image:
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No,
this isn't a Hubble shot. But this image was acquired
and processed just like the gorgeous Hubble telescope
images that we've come to love. To accomplish
this, the image was taken through specialized, narrowband
emission line filters. This information was then
"mapped" to the traditional red, green, and
blue channels of an RGB image. The greenish portions
of the image represent Hydrogen-alpha ionized gases.,
the bluish color represents
doubly ionized Oxygen gases, and the reddish areas represent singly ionized Sulfur gases. While
the stars glow heavily in the sulfur wavelength, there
is only a light concentration of it in the nebula, mostly
throughout the brighter portions.
Such
images, while obviously beautiful, have a real scientific
purpose. Because the colors are mapped specifically
to certain gases, it's easy to understand the concentrations
of ionizations and how (where) they interact with each
other.
Named
NASA's Astronomy Picture of the Day for March 24, 2006...coined,
"When Roses Aren't Red." See it <here>
on APOD.
To see this same data in CFHT-mapped
colors,
click
<here> For
NGC 2244 in regular RGB, click <here>
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Location:
Ballauer
Observatory near Azle, Texas and Date: November,
2005 to January 2006 Seeing:
Varied
Transparency: Varied
Scope/Mount: 12.5" RCOS
RC and Paramount ME
Camera: SBIG STL-6303e astro
CCD camera Filters: Custom Scientific 4.5nm Ha,
OIII, and SII spectral line filters.
Exposure Info: Mapped
color mosaic - SII/Ha/OIII - 90:210:60 minutes for left side and
90:150:90 minutes for right side (20 and 30 minute subexposures
unbinned)
Processing Information:
Calibration,
Registration, and DDP in CCDStack. Color mapping, cropping, color balance, levels/curves, sharpening, and
noise removal (Astronomy Tools/Pro Digital Software) in Photoshop CS.
Exposure Notes:
The SII data is mapped
to the red channel, Ha to green, and OIII to blue. Seeing
was exceptional for the left side of the mosaic, but poor for the
right. Interesting to note that despite similar conditions,
the left side is much cleaner than the right side despite having
less exposure time in Ha.
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rights reserved.
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