NGC 6729

NGC 6729 is a reflection and emission nebula located in the constellation Corona Australis, about 400 light-years from Earth. It is part of a dynamic star-forming region and is closely associated with the variable star R Coronae Australis. The nebula exhibits a distinctive fan-shaped structure, shaped by young stellar outflows and surrounding dust. NGC 6729 is an important target for studying the early stages of stellar evolution.