WLM
Wolf-Lundmark-Melotte I
Local
Group Galaxy in Cetus
Uploaded
12/15/07
This Local Group Galaxy
outlier is extremely difficult to image due to its low surface
brightness, extended size and low declination. Located on the
border of Cetus and Aquarius, this 11th magnitude object is 12
x 4 arcminutes in size and was first discovered in 1909 by Max
Wolf. Its nature as a galaxy was only established in 1926 by
Knut Lundmark and Philibert Jacques Melotte (1880-1961). Not
only is WLM at the frontier of the Local Group, but it is also
very isolated its nearest neighbor, the dwarf galaxy IC
1613, a full million light-years away. Quite elongated, with
a largest extension of more than 8,000 light years, WLM is about
12 times smaller than the Milky Way. Yet the discovery around
it of many outlying red stars suggests that even such galactic
minnows may have haloes and that WLM may be similar to our own
galaxy in age.
Imaging this object
is a challenge to say the least. Because it is very low on the
horizon, the seeing dominates the quality. Here, stars have been
resolved across the face of the galaxy, most dimmer than magnitude
20. A lack of obvious HII regions in the RGB data shows the galaxy
to be rather gas poor, however I do plan on some deep hydrogen
exposures to be certain.
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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: Meade DSI Pro w/Lumicon Newt Easy Guider
Exposure: LRGB = 80:20:20:20 (RGB Binned 2x2)
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: 30 F
CCD Temperature: -30 C
Image Processing Tools:
Maxim DL: Calibration, deblooming (Starizona Debloomer), aligning, stacking
PixInsight: Curves, Deconvolution, noise reduction
Photoshop CS2: Curves, Color Correction, Gradient removal (Grad Xterminator), Cleanup
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