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Dates & Location |
5th August 2018 - 9th August 2019 from the ICAstro
site, Alcalali then Oria, Spain. Elevation 1022 m |
Catalogue Identification(s) |
SH2-129 - the Flying Bat Nebula (red Ha) |
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Equipment Used | Tak FSQ106N at 530 mm focal length, F5.0. |
Where it is in space |
This field is approx 141 x 176 arcminutes - ie
~ 6 x 4 Moon diameters
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Acquisition | Remote
sessions using Splashtop control from Ravenshead, UK
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What it is | Discovered in 2011 by French astro-imager Nicolas Outters, the Squid Nebula's alluring bipolar shape is distinguished here by the telltale blue-green emission from doubly ionized oxygen atoms. Though apparently completely surrounded by the reddish hydrogen emission region Sh2-129, the true distance and nature of the Squid Nebula have been difficult to determine. Still, a recent investigation suggests Ou4 really does lie within SH2-129 some 2,300 light-years away. Consistent with that scenario, Ou4 would represent a spectacular outflow driven by HR8119, a triple system of hot, massive stars seen near the center of the nebula. If so, the truly giant Squid Nebula would physically be nearly 50 light-years across. loud. |
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Processing Methods |
All data reduction with CCDStack. Lum, RGB masters and RGB colour combine prepared in CCDStack. |
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