Teutsch 51
(Koposov 52; MWSC 693; FSR 0847; DSH J0553.8+2649)
0.83
UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
14.4 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Teutsch 51 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 88.463 | 26.834 | 0.233 | 0.536 | -0.32 | 16.329 |
| Otto et al. | 2026 | 88.464 | 26.83 | β | 0.55 | -0.34 | 17.6 |
| Guerco et al. | 2025 | 88.5 | 26.8 | 0.24 | 0.56 | -0.22 | 17.7 |
| Hunt & Reffert | 2024 | 88.464 | 26.83 | 0.236 | 0.538 | -0.317 | 13.463 |
| Cavallo et al. | 2024 | 88.471 | 26.821 | 0.226 | β | β | β |
| Hunt & Reffert | 2023 | 88.464 | 26.83 | 0.236 | 0.538 | -0.317 | 13.463 |
| Just et al. | 2023 | 88.45 | 26.831 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 88.463 | 26.834 | β | β | β | β |
| Netopil et al. | 2022 | 88.463 | 26.834 | β | β | β | 14.8 |
| Spina et al. | 2021 | 88.461 | 26.834 | 0.202 | 0.55 | -0.379 | β |
| Cantat-Gaudin et al. | 2020 | 88.463 | 26.834 | 0.216 | 0.545 | -0.345 | β |
| SΓ‘nchez et al. | 2020 | 88.467 | 26.83 | β | 0.504 | -0.399 | β |
| Donor et al. | 2020 | 88.46 | 26.83 | β | 0.62 | -0.29 | 17.7 |
| Zhong et al. | 2020 | 88.463 | 26.834 | β | 0.545 | -0.345 | 3.875 |
| Cantat-Gaudin & Anders | 2020 | 88.463 | 26.834 | 0.216 | 0.545 | -0.345 | β |
| Bica et al. | 2019 | 88.464 | 26.832 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 88.463 | 26.834 | 0.216 | 0.545 | -0.345 | β |
| Loktin & Popova | 2017 | 88.47 | 26.83 | β | 0.782 | -0.838 | β |
| Sampedro et al. | 2017 | 88.467 | 26.83 | 2.15 | -2.21 | β | β |
| Kharchenko et al. | 2016 | 88.45 | 26.831 | β | β | β | β |
| Kharchenko et al. | 2013 | 88.459 | 26.83 | β | 1.31 | -1.12 | β |
| Bukowiecki et al. | 2011 | 88.463 | 26.825 | β | β | β | β |
| Glushkova et al. | 2010 | 88.454 | 26.841 | β | β | β | β |
| Koposov et al. | 2008 | 88.454 | 26.841 | β | β | β | β |
| Kronberger et al. | 2006 | 88.466 | 26.83 | β | β | β | β |
| Dias et al. | 2002 | 88.467 | 26.83 | β | 1.31 | -1.12 | 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 | 4.08 | 3.25 | 2.12 | 676 | -0.330 | 1923 | β | 2 |
| Otto et al. | 2026 | β | β | β | 676 | -0.330(15) | β | β | β |
| Guerco et al. | 2025 | β | β | β | 680 | -0.360 | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2155(1) | β | β |
| Cavallo et al. | 2024 | 4.70 | 3.25 | β | 562 | -0.030 | β | β | β |
| Hunt & Reffert | 2023 | 3.76 | 3.17 | 2.12 | 753 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 531 | β | 327 | β | β |
| Spina et al. | 2022 | β | β | β | β | -0.330 | β | β | β |
| Jadhav & Subramaniam | 2021 | 4.68 | 2.62 | β | 676 | β | 1923 | β | 2(1) |
| Netopil et al. | 2022 | 4.67(1) | β | β | 676 | -0.330(1) | β | β | β |
| Spina et al. | 2021 | 3.93 | β | β | 676 | -0.319(20) | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.68 | 2.62 | β | 676 | β | β | β | β |
| Kounkel et al. | 2020 | 4.50 | 2.76 | β | 1148 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.330 | β | β | β |
| Zhong et al. | 2020 | 4.08(1) | 4.01 | β | 8725 | -0.017 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.08 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.08 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 6.36 | 3.44 | β | 245 | β | β | β | β |
| Kharchenko et al. | 2016 | 3.79 | 4.01 | β | 531 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.79 | 4.01 | β | 531 | β | β | β | β |
| Bukowiecki et al. | 2011 | 4.69(1) | 2.90 | β | 1122 | β | β | β | β |
| Glushkova et al. | 2010 | 2.90 | 3.25 | β | 891 | β | β | β | β |
| Koposov et al. | 2008 | 2.90 | 3.25 | β | 891 | β | β | β | β |
| Kronberger et al. | 2006 | 3.30 | 3.34 | β | 794 | β | β | β | β |
| Dias et al. | 2002 | 3.30 | 3.34 | β | 794 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.26 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.26 (50th percentile).