Cederblad 51

Cederblad 51
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Cederblad 51

Cederblad 51 is part of Sharpless 2-264 in what is commonly known as Orion's head. It is also known as the Lambda Orionis Ring, is a molecular cloud and H II region, which can be seen in the northern region of the Orion Molecular Cloud Complex an area of large hot new star formation.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
CHI-2 & CHI-4
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL16803
Location ..........................................................................................................................................................................................................................
Location
El Sauce observatory, Chile
Date of observation ..........................................................................................................................................................................................................................
Date of observation
13th February 2022
Filters ..........................................................................................................................................................................................................................
Filters
LRGB
Processing ..........................................................................................................................................................................................................................
Processing
Integration and background subtraction in Pixinsight, star reduction, levels and clarity in Affinity photo.
Credits ..........................................................................................................................................................................................................................
Credits
N.Streeter Data set Nik Szymanek
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