CWNU 3579 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~15.48 kpc) differs significantly from the median photometric distance (~9.55 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	111.685	-27.349	0.065	-0.999	1.688	149.327
He et al.	2023	111.68	-27.36	0.097	-1.011	1.738	149.33

💡 Note: The UCC values are estimated from its identified members.