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M33
- The Pinwheel Galaxy
Spiral
Galaxy in Triangulum
Uploaded
12/3/05
How does one begin to describe
such an incredible object in mere words? This image of the Pinwheel
Galaxy is my deepest image yet of this splendor, and from an
image processing standpoint required developing some all new
techniques. The last
time I
shot this galaxy with a CCD was in 2001 and used my ST7E. Now
lets get down to the details:
The Galaxy
Located in a
relatively star poor constellation, M33 has an integrated photographic
magnitude of 6.3, but is spread out over a degree of sky, and
thus is low surface brightness. Despite this, it is a very easy
naked eye object on any clear night, when Triangulum rides high
in the fall and early winter skies. An interesting fact is that
the B-V index is .55, which is getting quite reddish. You can
see in my image above why that would be the case, the entire
galaxy is covered with an enormous amount of red hydrogen (HII
regions), and the blue part of the arms does not really start
until a fair distance out from the center, thus the more yellow
core is the dominant light source here. This galaxy actually
has a measurable inclination, of about 4 degrees and is classed
as an SA(s)cd galaxy.
There are literally
hundreds of reddish - pink HII regions in this image. While most
atlases identify maybe half a dozen of the more prominent ones,
Simbad and the Aladin online Atlas has thousands of objects.
Look closely and you will see that a majority of them surround
blue stars and associations. When I first put this image together,
I couldnt believe how many HII regions contained the source of
thier illumination, mostly hot O/B stars and clusters. I invite
you to explore the largest image and take in the knots, faint
tendrils and wreaths of nebulosity, and countless resolved blue
supergiants here seen in another galaxy.
Processing
2 hours of unfiltered
Luminance data (IR included), and one hour of H-alpha data were
combined to make a detailed L channel. This was combined with
one hour of RGB data in Photoshop using layers, with the RGB
layer set to "color". The H-alpha data was next processed
separately, and the stars removed by subtracting the blue channel.
The color was added by using the color of the brightest nebulosities
in the RGB data to tint the image. Next, this final H-alpha only
image was layered in PS with the LRGB created earlier and combined
with Lighten.
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Instrument: 12.5" f/5 Home made Newtonian
Platform: Astrophysics 1200 QMD
CCD Camera: SBIG 10XME NABG with Enhanced Cooling
Guider: SBIG ST4
Exposure: HaLRGB = 60:170:20:20:20 (RGB Binned 2x2)
RGB Combine Ratio: 1: 1.05: 1.11
Filters: AstroDon RGB Tricolor, H-Alpha, Clear
Location: Payson, Arizona
Elevation: 5150 ft.
Sky: Seeing FWHM = 6.5 arcsec (Maxim DL - 10min subframe), Transparency 8/10
Outside Temperature: 40 F
CCD Temperature: -30 C
Processing Tools: Maxim DL, Photoshop, PixInsight, CCDOps Debloomer.
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