Astronomy and Space

CX330

CX330 (also known as CXOGBS J173643.8-282122) is an extremely isolated young stellar object (YSO) located in the central bulge of the Milky Way, approximately 25,000 light-years from Earth. Identified in 2009 through its X-ray emission, it is the most isolated known young star, situated over 1,000 light-years from the nearest star-forming region (nearest star-forming region from CX330 is NGC 6383 followed by Pipe Nebula and Corona Australis Molecular Cloud). CX330 is a FU Orionis-type protostar undergoing episodic accretion outbursts, making it a unique laboratory for studying star formation in low-density environments.

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See also

• ▸Error detection and correction
• ▸Aretino and Charles V's Ambassador
• ▸Eta Corvi

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