NGC 6729

NGC 6729
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NGC 6729

This is an image of NGC 6729. It is an emission and reflection nebula about 425 light years away in the constellation Corona Austrailis. It is one of the closest star forming regions to earth.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
Planewave CDK24
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600M
Location ..........................................................................................................................................................................................................................
Location
Rio Hurtado, Chile
Date of observation ..........................................................................................................................................................................................................................
Date of observation
25 August 2023
Filters ..........................................................................................................................................................................................................................
Filters
Astrodon 2GEN, LRGB
Processing ..........................................................................................................................................................................................................................
Processing
Pixinsight and Photoshop
Credits ..........................................................................................................................................................................................................................
Credits
Bernard Miller/Telescope Live
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