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Instrument |
12.5" RCOS @
~f/9 (2880 mm fl) 1.28 arcsec / pixel. Zoomify image scale is
1.28 to 3.33 arcsec / pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/ internal filter wheel, AstroDon Gen I Filters |
Acquisition Data |
6/19/2010 to 8/5/2010
Chino Valley, AZ... with CCDAutoPilot3 & CCDSoft, AOL guided |
Exposure |
Hα
600 min. (20 x 30 min. bin 2x2)
OIII 660 min. (22 x 30 min. bin 2x2)
RGB 225 min. (
5 x 15 min each, bin 2x2)
Hα
[OIII + 20%Hα]
[OIII + 20% Hα]
and an overlay of RGB stars colors.
Click
here for an Ha filtered b/w version. |
Software |
-
CCDSoft, CCDStack,
Photoshop CS w/ the Fits Liberator plugin. Noel Carboni's actions.
-
eXcalibrator for (b-v), (v-r) star color calibration, using 26
stars from the NOMAD1 database.
-
PixFix32 (pre-beta) to
repair hot/cold pixels and column defects.
-
CCDStack to calibrate,
register, normalize, data reject, combine the sub exposures.
-
PhotoShop for color
combine &
on-linear stretching.
|
Comment |
North is to top.
NGC 6888, the Crescent
Nebula, is located the constellation Cygnus at a distance of about
5,000 light-years. The nebula is created by the bright central star,
HD 192163. About 400,000 years ago, the star ejected material, when
it became a red giant. Then, about 150,000 years later, HD 192163
shed its outer envelope into a strong stellar wind, and became a
Wolf-Rayet star (WR 136). The second explosion eventually over took
the previous ejected gas. This collision formed and lit up the
nebula we see today. Wr 136 is expected to end its life with a
supernova explosion, sometime in the next million years.
This synthetic color
image was created by mapping Ha data to red and OIII filtered data
to green and blue. This creates an image with hydrogen gas shown as
red and doubly
ionized oxygen is teal.
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