Teutsch 13 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

(*): The parallax distance estimate (~5.60 kpc) differs significantly from the median photometric distance (~4.24 kpc).

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	100.98	1.407	0.179	-0.143	0.515	–
Almeida et al.	2025	100.981	1.413	–	–	–	–
Hunt & Reffert	2024	100.976	1.407	0.171	-0.13	0.452	100.392
Celli et al.	2024	100.979	1.403	–	–	–	–
Cavallo et al.	2024	100.978	1.38	0.173	–	–	–
Hunt & Reffert	2023	100.976	1.407	0.171	-0.13	0.452	100.392
Almeida et al.	2023	100.979	1.414	–	–	–	–
Just et al.	2023	100.972	1.397	–	–	–	–
Dias et al.	2021	100.981	1.413	0.166	-0.122	0.545	–
Cantat-Gaudin et al.	2020	100.984	1.404	0.155	-0.097	0.518	–
Cantat-Gaudin & Anders	2020	100.984	1.404	0.155	-0.097	0.518	–
Bica et al.	2019	100.975	1.396	–	–	–	–
Cantat-Gaudin et al.	2018	100.984	1.404	0.155	-0.097	0.518	–
Loktin & Popova	2017	100.98	1.406	–	-0.476	-1.093	–
Kharchenko et al.	2016	100.972	1.397	–	–	–	–
Dias et al.	2014	100.979	1.405	–	-0.92	-1.64	–
Kharchenko et al.	2013	100.98	1.395	–	-2.64	-3.72	–
Kronberger et al.	2006	100.979	1.403	–	–	–	–
Dias et al.	2002	100.979	1.405	–	-0.92	-1.64	–

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