Teutsch 124
(MWSC 3307; DSH J2018.3+3112)
0.55
UTI
0.37
CN
0.25
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
1.4 [arcmin]
- CN 0.37 Poorly populated
- Cdens 0.25 Loose
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 124 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a very large* distance, below the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~13.37 kpc) differs significantly from the median photometric distance (~2.25 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Very high extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 304.575 | 31.217 | 0.075 | -3.067 | -4.506 | -34.582 |
| Hu & Soubiran | 2025 | 304.572 | 31.212 | â | â | â | â |
| Hunt & Reffert | 2024 | 304.576 | 31.21 | 0.079 | -3.07 | -4.538 | -34.417 |
| Cavallo et al. | 2024 | 304.572 | 31.212 | 0.08 | â | â | â |
| Hunt & Reffert | 2023 | 304.576 | 31.21 | 0.079 | -3.07 | -4.538 | -34.417 |
| Just et al. | 2023 | 304.582 | 31.207 | â | â | â | â |
| Bica et al. | 2019 | 304.592 | 31.213 | â | â | â | â |
| Loktin & Popova | 2017 | 304.59 | 31.206 | â | -1.052 | -1.64 | â |
| Kharchenko et al. | 2016 | 304.582 | 31.207 | â | â | â | â |
| Dias et al. | 2014 | 304.587 | 31.206 | â | 0.34 | -2.77 | â |
| Kharchenko et al. | 2013 | 304.587 | 31.21 | â | -2.85 | -5.33 | â |
| Kronberger et al. | 2006 | 304.588 | 31.212 | â | â | â | â |
| Dias et al. | 2002 | 304.587 | 31.206 | â | 0.34 | -2.77 | â |
đĄ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.090* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 5021* | â | â |
| Cavallo et al. | 2024 | 5.70 | 3.05 | â | 7943 | 0.590 | â | â | â |
| Hunt & Reffert | 2023 | 10.26 | 5.19 | 2.04 | 492 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2483 | â | 204 | â | â |
| Loktin & Popova | 2017 | 2.40 | 1.84 | â | 955 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.10 | 5.64 | â | 2483 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.10 | 5.64 | â | 2483 | â | â | â | â |
| Dias et al. | 2002 | 0.84 | 5.64 | â | 6918 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.