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Click the image for a larger view.
(2000 x 1500 1.37 MB)
Instrument |
Takahashi FSQ-106ED @
f/5.0 (530 mm F.L.) Captured at 2.1 arcsec/pixel. Shown at
3.48 and 9.27 arcsec/pixel. |
Mount |
Losmandy G11 with Gemini L4 v1.0 |
Camera |
SBIG STF-8300M Self
Guiding Package w/ mono ST-i, using Baader RGB filters. |
Acquisition Data |
1/22/2014
to 2/21/2014 Chino Valley, AZ... with CCDAutoPilot5 & CCDSoft. |
Exposure |
Lum |
240 min. (16 x
15 min. each bin 1x1) |
Red |
105 min. (7 x
15 min. each bin 1x1) |
Green
|
120 min. (8 x 15 min. each bin 1x1)
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Blue
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135 min. (9 x 15 min. each bin 1x1)
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Software & Processing Notes |
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CCDSoft, CCDStack, PixInsight
and Photoshop CS6.
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No SDSS stars were
available for color balancing, so a standard image-train color
calibration was used, as determined by
eXcalibrator
v4.2, and then adjusted for altitude extinction.
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CCDStack to
calibrate, register, normalize, data reject, combine the sub
exposures and to create the RGB
image.
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PixInsight for
gradient removal and initial non-linear stretching.
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PhotoShop for LRGB
combine and final touch-up.
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Noiseware 5, a
PhotoShop plug-in.
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Comment |
North is to the right.
At a distance of about 1000 light-years, this beautiful molecular
cloud is found at the very northeast corner of the constellation
Aries. Three blue reflection nebulae, vdB13, 16 and 17, highlight
the image. VdB 17 is also catalogued as NGC 1333. Although
reflection nebulae are usually blue, the image shows two
relatively rare yellow reflection nebula.
Also shown are several dark nebulae as identified by the Aladin Sky Atlas and catalogued by Beverly Lynds and Edward Barnard.
Scattered throughout the image are many HH objects. The two
groupings, at the upper right, are the most interesting. In the
1940s, George Herbig and Guillermo Haro independently studied and
identified these objects as a distinct type of the emission nebula.
The nebulae are associated with newly born stars. Several are often
seen around a single star and aligned with star's rotational axis. |
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