NGC 6888 - Crescent and Soap Bubble
This area within the greater Sadr region in the constellation Cygnus contains the Crescent nebula - the product of the tremendous stellar winds of a Wolf-Rayet star. These relatively rare stars are massive, young, and highly luminous. Gasses cast off during formation of the star are overtaken by intense radiation and fast stellar winds causing a shock wave to form. Here, hydrogen gas (red) is surrounded by an envelope of oxygen gas (blue). Also seen in this area is the Soap Bubble, a recently discovered, nearly perfectly spherical faint outgassing from a dying star (above and left of center).
Acquisition Details
Imaging telescope: Stellarvue SV105 APO
Imaging camera: QSI 683 wsg-8
Mount: Orion Atlas EQ-G (belt mod)
Guiding camera: Loadestar 2
Software: Main Sequence Software Seqence Generator Pro, Deep Sky Stacker (DSS), Photoshop CC, PhD Guiding 2
Resolution: 6406x4906
Dates: July 3, 2016, Aug. 22, Aug. 23, 2016
Frames:
Ha 1.25" 7nm: 24x1200" -20C bin 1x1
O3 1.25" 8.5nm: 25x1200" -20C bin 1x1
S2 1.25" 8nm: 27x1200" -20C bin 1x1
Integration: 25.3 hours
Darks: ~50
Flats: ~50
Bias: ~100
Bortle Dark-Sky Scale: 5.00
RA center: 303.527 degrees
DEC center: 38.104 degrees
Pixel scale: 1.6 arcsec/pixel
Sky Map
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