RCW - 38

RCW - 38
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RCW - 38

RCW 38 is an HII region containing a massive star cluster located approximately 5,500 light years away from Earth in the direction of the constellation Vela. The stars were very recently formed, and are still enshrouded within the dark cloud in which they were born.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
ASA 500N
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL 16803
Location ..........................................................................................................................................................................................................................
Location
Río Hurtado, Coquimbo Region, Chile
Date of observation ..........................................................................................................................................................................................................................
Date of observation
14 April 2021
Filters ..........................................................................................................................................................................................................................
Filters
HSO
Processing ..........................................................................................................................................................................................................................
Processing
Affinity Photo | JR Astrophotography Macro | Nik Collection
Credits ..........................................................................................................................................................................................................................
Credits
The observations were taken by Ian Howarth.
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