Teutsch 10
(Koposov 49; MWSC 661; DSH J0544.3+2848; FSR 0829)
0.83
UTI
0.66
CN
1.0
Cdens
0.5
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
21.3 [N/pc2]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Teutsch 10 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 86.095 | 28.822 | 0.324 | 0.812 | -1.94 | 1.89 |
| Hu & Soubiran | 2025 | 86.084 | 28.826 | â | â | â | â |
| Almeida et al. | 2025 | 86.089 | 28.84 | â | â | â | â |
| Hunt & Reffert | 2024 | 86.098 | 28.817 | 0.308 | 0.825 | -1.949 | 3.558 |
| Cavallo et al. | 2024 | 86.084 | 28.827 | 0.307 | â | â | â |
| Hunt & Reffert | 2023 | 86.098 | 28.817 | 0.308 | 0.825 | -1.949 | 3.558 |
| Just et al. | 2023 | 86.098 | 28.826 | â | â | â | â |
| Dias et al. | 2021 | 86.089 | 28.84 | 0.331 | 0.87 | -1.917 | 0.556 |
| Cantat-Gaudin et al. | 2020 | 86.096 | 28.828 | 0.319 | 0.834 | -1.892 | â |
| Donor et al. | 2020 | 86.108 | 28.825 | â | 0.84 | -1.9 | 5.6 |
| Cantat-Gaudin & Anders | 2020 | 86.096 | 28.828 | 0.319 | 0.834 | -1.892 | â |
| Soubiran et al. | 2018 | 86.096 | 28.828 | â | â | â | 1.72 |
| Bica et al. | 2019 | 86.099 | 28.819 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 86.096 | 28.828 | 0.319 | 0.834 | -1.892 | â |
| Loktin & Popova | 2017 | 86.085 | 28.821 | â | 0.743 | -0.282 | â |
| Kharchenko et al. | 2016 | 86.098 | 28.826 | â | â | â | â |
| Dias et al. | 2014 | 86.092 | 28.82 | â | -2.55 | -1.43 | â |
| Kharchenko et al. | 2013 | 86.107 | 28.825 | â | 2.1 | -0.59 | â |
| Kharchenko et al. | 2012 | 86.107 | 28.825 | â | 2.1 | -0.59 | â |
| Glushkova et al. | 2010 | 86.093 | 28.82 | â | â | â | â |
| Koposov et al. | 2008 | 86.093 | 28.82 | â | â | â | â |
| Kronberger et al. | 2006 | 86.096 | 28.815 | â | â | â | â |
| Dias et al. | 2002 | 86.092 | 28.82 | â | -2.55 | -1.41 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.6 | 2.58 | 2.02 | 239 | -0.283 | 439 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.310(5) | â | â | â |
| Almeida et al. | 2025 | 2.32 | 2.57 | â | 289 | â | 395 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 858(1) | â | â |
| Cavallo et al. | 2024 | 2.84 | 2.63 | â | 575 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 2.89 | 2.59 | 2.02 | 239 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 63 | â | 439 | â | â |
| Dias et al. | 2021 | 2.32 | 2.57 | â | 289 | -0.296 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.45 | 1.81 | â | 617 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.270 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.88 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.88 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.88 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 4.58 | 2.38 | â | 195 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.60 | 3.16 | â | 63 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.60 | 3.16 | â | 63 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.60 | 3.16 | â | 63 | â | â | â | â |
| Glushkova et al. | 2010 | 2.00 | 1.30 | â | 1413 | â | â | â | â |
| Koposov et al. | 2008 | 2.00 | 1.30 | â | 1413 | â | â | â | â |
| Dias et al. | 2002 | 2.60 | 3.13 | â | 32 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.