NGC 2170 - Angel nebula

NGC 2170 - Angel nebula
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NGC 2170 - Angel nebula

The Angel Nebula is a reflection nebula located approximately 2,700 light-years away in the equatorial constellation Monoceros (the Unicorn). It is part of Monoceros R2, one of the closest massive star forming regions to the Sun.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
CHI-1 - Planewave CDK24
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL 9000
Location ..........................................................................................................................................................................................................................
Location
EL SAUCE OBSERVATORY, CHILE
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Feb - Mar 2024
Filters ..........................................................................................................................................................................................................................
Filters
LRGB
Processing ..........................................................................................................................................................................................................................
Processing
Siril, Starnet++, Affinity Photo2, GraXpert
Credits ..........................................................................................................................................................................................................................
Credits
Tomas Samek, data obtained at TelescopeLive
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