Teutsch 182
(UBC 6)
0.77
UTI
0.85
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
20.1 [N/pc2]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 182 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 344.032 | 51.177 | 0.696 | -4.623 | -4.946 | -33.086 |
| Li et al. | 2025 | 344.01 | 51.187 | 0.676 | -4.644 | -4.896 | â |
| Hu & Soubiran | 2025 | 343.991 | 51.178 | â | â | â | â |
| Zhang et al. | 2024 | 344.072 | 51.145 | â | â | â | â |
| Hunt & Reffert | 2024 | 344.072 | 51.145 | 0.699 | -4.621 | -4.963 | -32.065 |
| Cavallo et al. | 2024 | 343.991 | 51.178 | 0.699 | â | â | â |
| Hunt & Reffert | 2023 | 344.072 | 51.145 | 0.699 | -4.621 | -4.963 | -32.065 |
| Tarricq et al. | 2022 | 344.045 | 51.159 | 0.692 | -4.622 | -4.958 | â |
| Cantat-Gaudin et al. | 2020 | 344.01 | 51.187 | 0.676 | -4.644 | -4.896 | â |
| Cantat-Gaudin & Anders | 2020 | 344.01 | 51.187 | 0.676 | -4.644 | -4.896 | â |
| Bica et al. | 2019 | 343.94 | 51.199 | â | â | â | â |
| Castro-Ginard et al. | 2018 | 343.952 | 51.199 | 0.674 | -4.646 | -4.904 | -31.64 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.415 | 0.51 | 0.46 | 912 | -0.017 | 923 | â | â |
| Li et al. | 2025 | 1.36 | 0.47 | â | 1199 | -0.038 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.120(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.004(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 923(1) | â | â |
| Cavallo et al. | 2024 | 1.41 | 0.55 | â | 912 | 0.330 | â | â | â |
| Hunt & Reffert | 2023 | 1.36 | 0.25 | 0.46 | 966 | â | â | â | â |
| Tarricq et al. | 2022 | 1.44 | â | â | 794 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.49 | 0.64 | â | 741 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.42 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.