FSR 0255 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~2.26 kpc) differs significantly from the median photometric distance (~1.23 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	–	308.987	44.372	0.442	-3.006	-4.042	-26.656
Bica et al.	2019	308.973	44.327	–	–	–	–
Froebrich et al.	2007	308.971	44.325	–	–	–	–
Dias et al.	2002	308.971	44.325	–	-2.17	-3.66	–

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