FSR 0759 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~5.69 kpc) differs significantly from the median photometric distance (~3.80 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	–	75.308	35.789	0.176	0.829	-0.416	7.081
Bica et al.	2019	75.295	35.798	–	–	–	–
Froebrich et al.	2007	75.292	35.795	–	–	–	–
Dias et al.	2002	75.292	35.795	–	6.24	-4.1	–

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