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M13
Click the image for 3/4 scale (0.85 arcsec/pixel)
uncropped display.
Instrument |
12.5" RCOS @
~f/9 (2880 mm fl) 0.643 arcsec / pixel. Shown
resampled to 2.28 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Filters |
Acquisition Data |
5/4/2008 to 5/26/2008
Chino Valley... with CCDAutoPilot3 |
Exposure |
Lum
165 min. (33 x 5 min. bin 1x1)
RGB
180 min. (12 x 5 min. bin 2x2) each |
Software |
-
CCDSoft, CCDStack, PixInsight
and Photoshop CS6.
-
eXcalibrator v4.25
for (g:r) color balancing, using 68 stars from the SDSS-DR9
database.
-
CCDSoft for calibrartion
-
CCDStack to
register, normalize, data reject, combine the sub
exposures and create the RGB
image.
-
PixInsight for
gradient removal and initial non-linear stretching.
-
PhotoShop for the
LRGB
combine and final touch-up.
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Comment |
North is to the top.
M13, the Great Globular Cluster in Hercules, is a system of stars
numbering in the hundreds of thousands. It is one of the
brightest globular star clusters in the northern sky. At a distance
of 25,000 light-years, the cluster stars crowd into a region 150
light-years in diameter, but approaching the cluster core over 100
stars would be contained in a cube just 3 light-years on a side. For
comparison, the closest star to the Sun is over 4 light-years away.
The orange stars are red giants, which are typically 2000 times
brighter than our sun. Also visible are many hot blues stars
known as "blue stragglers." The most likely explanation for blue
stragglers seems to be that they are the result of stellar
collisions or mass transfer from another star.
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