NGC 6165

NGC 6165
0

NGC 6165

NGC 6164-5 is a bipolar nebula surrounding the star HD 148937.
Although the nebula was believed to represent a planetary nebula, it is now understood to represent a shell-like ejected nebula, formed by the winds of its young central star.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
CHI-1 Planewave CDK24
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL16803
Location ..........................................................................................................................................................................................................................
Location
Chile -70.76300° E -30.47253° N
Date of observation ..........................................................................................................................................................................................................................
Date of observation
19th Feb 2022
Filters ..........................................................................................................................................................................................................................
Filters
SHO
Processing ..........................................................................................................................................................................................................................
Processing
Pixinsight and Photoshop
Credits ..........................................................................................................................................................................................................................
Credits
P Yates
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