Ryu 614 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very large 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 7 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	–	273.067	-23.566	0.095	-4.459	-7.312	–
Bica et al.	2019	273.058	-23.567	–	–	–	–

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