Dolidze 45 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.

(*): The parallax distance estimate (~7.36 kpc) differs significantly from the median photometric distance (~2.46 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	–	317.707	37.565	0.136	-2.213	-3.619	–
Loktin & Popova	2017	317.7	37.534	–	-0.684	-0.667	–
Dias et al.	2014	317.692	37.574	–	-0.12	-3.08	–
Dias et al.	2002	317.692	37.574	–	-0.12	-3.08	–

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