Stock 19 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low 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 9 years.

(*): The parallax distance estimate (~5.08 kpc) differs significantly from the median photometric distance (~1.57 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	–	1.183	56.058	0.197	-2.167	-1.717	-72.953
Loktin & Popova	2017	1.17	56.083	–	-1.912	-4.367	–
Dias et al.	2014	1.171	56.083	–	1.43	-2.04	–
Dias et al.	2002	1.171	56.083	–	1.43	-2.04	–

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