NGC 2626

NGC 2626
NGC2626 V2
0

NGC 2626

NGC 2626 is a reflection nebula, emission nebula, and absorption nebula in the constellation Vela. It is mostly illuminated by B1 star CD-40 4432 and ionized by the O8 quadruple star system HD 73882, together with other stars. It is about 3,200 light-years away from Earth.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
CHI-1-CMOS
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600M
Location ..........................................................................................................................................................................................................................
Location
Río Hurtado Valley, Chile
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Observation Bundle
Filters ..........................................................................................................................................................................................................................
Filters
LRGB
Processing ..........................................................................................................................................................................................................................
Processing
PixInsight WBPP GraXpert GHS BXT NXT SXT
Credits ..........................................................................................................................................................................................................................
Credits
Ian Baber.
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