Teutsch 61
(SAI 78; MWSC 1270; DSH J0734.6-1947; FSR 1266; FoF 936)
0.83
UTI
0.55
CN
1.0
Cdens
0.62
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
14.4 [N/pc2]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Teutsch 61 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, young 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 | 99999β | 113.66 | -19.792 | 0.316 | -2.293 | 3.164 | β |
| Li et al. | 2025 | 113.661 | -19.793 | 0.31 | -2.277 | 3.145 | β |
| Almeida et al. | 2025 | 113.663 | -19.787 | β | β | β | β |
| Hunt & Reffert | 2024 | 113.671 | -19.794 | 0.333 | -2.286 | 3.183 | β |
| Cavallo et al. | 2024 | 113.671 | -19.781 | 0.332 | β | β | β |
| Hunt & Reffert | 2023 | 113.671 | -19.794 | 0.333 | -2.286 | 3.183 | β |
| Almeida et al. | 2023 | 113.662 | -19.788 | β | β | β | β |
| Just et al. | 2023 | 113.657 | -19.798 | β | β | β | β |
| Dias et al. | 2021 | 113.663 | -19.787 | 0.301 | -2.304 | 3.143 | β |
| Cantat-Gaudin et al. | 2020 | 113.661 | -19.793 | 0.31 | -2.277 | 3.145 | β |
| SΓ‘nchez et al. | 2020 | 113.667 | -19.79 | β | -2.393 | 2.984 | β |
| Cantat-Gaudin & Anders | 2020 | 113.661 | -19.793 | 0.31 | -2.277 | 3.145 | β |
| Liu & Pang | 2019 | 113.663 | -19.781 | 0.307 | -2.276 | 3.076 | β |
| Bossini et al. | 2019 | 113.661 | -19.793 | β | β | β | β |
| Bica et al. | 2019 | 113.659 | -19.799 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 113.661 | -19.793 | 0.31 | -2.277 | 3.145 | β |
| Loktin & Popova | 2017 | 113.655 | -19.797 | β | -3.607 | 4.92 | β |
| Kharchenko et al. | 2016 | 113.657 | -19.798 | β | β | β | β |
| Kharchenko et al. | 2013 | 113.662 | -19.8 | β | -2.4 | 4.89 | β |
| Glushkova et al. | 2010 | 113.666 | -19.79 | β | β | β | β |
| Kronberger et al. | 2006 | 113.664 | -19.799 | β | β | β | β |
| Dias et al. | 2002 | 113.667 | -19.79 | β | -0.9 | 1.94 | β |
π‘ 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 | 99999β | 2.56 | 1.76 | 1.35 | 46 | 0.020 | 316 | 0.54 | β |
| Li et al. | 2025 | 2.56 | 1.89 | β | 43 | 0.040 | β | β | β |
| Almeida et al. | 2025 | 2.45 | 1.95 | β | 52 | β | 283 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 448(1) | β | β |
| Cavallo et al. | 2024 | 2.81 | 2.00 | β | 40 | 0.250 | β | β | β |
| Hunt & Reffert | 2023 | 2.74 | 1.90 | 1.35 | 36 | β | β | β | β |
| Almeida et al. | 2023 | 2.45 | 2.01 | β | 27 | -0.113 | 349(1) | 0.54 | β |
| Just et al. | 2023 | β | β | β | 164 | β | 73 | β | β |
| Dias et al. | 2021 | 2.45 | 1.95 | β | 52 | -0.013 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.98 | 1.64 | β | 46 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.95 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 6 | 0.500 | β | β | β |
| Bossini et al. | 2019 | 3.24 | 1.76 | β | 49 | 0.000 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.95 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.29 | 0.86 | β | 813 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.00 | 1.62 | β | 164 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.00 | 1.62 | β | 164 | β | β | β | β |
| Glushkova et al. | 2010 | 1.92 | 1.71 | β | 9 | β | β | β | β |
| Dias et al. | 2002 | 1.92 | 1.71 | β | 9 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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