FSR 0849 is a sparse, moderately dense object of very low C3 quality. Its parallax locates it at a relatively close^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 16 years.

(*): The parallax distance estimate (~1.77 kpc) differs significantly from the median photometric distance (~1.06 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	–	87.814	25.77	0.565	0.101	-2.01	18.178
Glushkova et al.	2010	87.796	25.778	–	–	–	–
Froebrich et al.	2007	87.804	25.772	–	–	–	–
Dias et al.	2002	87.804	25.772	–	1.35	-3.26	–

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