Collinder 345 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 8 years.

⚠️ 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	99999–	266.156	-33.864	0.352	0.574	-1.354	-49.619
Dias et al.	2018	–	–	–	-0.53	-3.26	–
Sampedro et al.	2017	266.146	-33.867	–	0.29	-1.02	–
Dias et al.	2014	266.146	-33.867	–	0.6	-1.38	–
Lynga	1987	266.146	-33.746	–	–	–	–

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