Teutsch 125

(FSR 0360; MWSC 3597; DSH J2212.5+5851)

0.62 UTI

0.27

C_N

1.0

C_dens

0.25

C_C3

0.79

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 27

Radius (P>50% members) 2.5 [arcmin]

C_N 0.27 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.79 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 SciX 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

Teutsch 125 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.

Relatively close Moderate extinction Metal-rich Intermediate age

Cavallo et al. (2024): Bronze sample.

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	333.317	58.939	0.471	-3.851	-2.862	-35.093
Hunt & Reffert	2024	333.299	58.941	0.471	-3.842	-2.897	-35.076
Celli et al.	2024	333.132	58.853	–	–	–	–
Cavallo et al.	2024	333.394	58.983	0.469	–	–	–
Hunt & Reffert	2023	333.299	58.941	0.471	-3.842	-2.897	-35.076
Just et al.	2023	333.285	58.973	–	–	–	–
Cantat-Gaudin et al.	2020	333.316	58.939	0.469	-3.867	-2.78	–
Bica et al.	2019	333.131	58.846	–	–	–	–
Cantat-Gaudin et al.	2018	333.316	58.939	0.469	-3.867	-2.78	–
Kharchenko et al.	2016	333.285	58.973	–	–	–	–
Kharchenko et al.	2013	333.291	58.977	–	-3.72	-0.74	–
Kharchenko et al.	2012	333.291	58.977	–	-3.72	-0.74	–
Froebrich et al.	2007	333.262	58.989	–	–	–	–
Kronberger et al.	2006	333.132	58.853	–	–	–	–

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

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Hunt & Reffert	2024	–	–	–	–	–	402*	–	–
Celli et al.	2024	–	–	–	9	–	247	–	–
Cavallo et al.	2024	2.37	3.25	–	78	0.670	–	–	–
Hunt & Reffert	2023	2.04	3.74	2.82	12	–	–	–	–
Just et al.	2023	–	–	–	1259	–	37	–	–
Cantat-Gaudin et al.	2020	2.11	2.72	–	9	–	–	–	–
Cantat-Gaudin et al.	2018	2.01	–	–	–	–	–	–	–
Kharchenko et al.	2016	1.45	2.42	–	1259	–	–	–	–
Kharchenko et al.	2013	1.45	2.42	–	1259	–	–	–	–
Kharchenko et al.	2012	1.45	2.42	–	1259	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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💡 Note: How are the galactocentric plots generated? See FAQ.