Teutsch 74
(SAI 144; MWSC 3558; DSH J2145.6+5805)
0.91
UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.0 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Teutsch 74 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, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Distant
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 | β | 326.42 | 58.095 | 0.2 | -3.231 | -3.133 | -72.416 |
| Hu & Soubiran | 2025 | 326.426 | 58.1 | β | β | β | β |
| Almeida et al. | 2025 | 326.433 | 58.096 | β | β | β | β |
| Hunt & Reffert | 2024 | 326.417 | 58.095 | 0.201 | -3.224 | -3.128 | -71.7 |
| Cavallo et al. | 2024 | 326.426 | 58.1 | 0.203 | β | β | β |
| Hunt & Reffert | 2023 | 326.417 | 58.095 | 0.201 | -3.224 | -3.128 | -71.7 |
| Just et al. | 2023 | 326.411 | 58.092 | β | β | β | β |
| Dias et al. | 2021 | 326.433 | 58.096 | 0.212 | -3.226 | -3.068 | -71.231 |
| Cantat-Gaudin et al. | 2020 | 326.422 | 58.097 | 0.218 | -3.244 | -3.064 | β |
| SΓ‘nchez et al. | 2020 | 326.433 | 58.084 | β | -3.333 | -3.076 | β |
| Cantat-Gaudin & Anders | 2020 | 326.422 | 58.097 | 0.218 | -3.244 | -3.064 | β |
| Soubiran et al. | 2018 | 326.422 | 58.097 | β | β | β | -71.16 |
| Bica et al. | 2019 | 326.411 | 58.092 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 326.422 | 58.097 | 0.218 | -3.244 | -3.064 | β |
| Loktin & Popova | 2017 | 326.43 | 58.084 | β | 3.276 | -5.35 | β |
| Kharchenko et al. | 2016 | 326.411 | 58.092 | β | β | β | β |
| Dias et al. | 2014 | 326.433 | 58.084 | β | 1.13 | -2.65 | β |
| Kharchenko et al. | 2013 | 326.415 | 58.095 | β | 3.31 | -3.58 | β |
| Kharchenko et al. | 2012 | 326.415 | 58.095 | β | 3.31 | -3.58 | β |
| Glushkova et al. | 2010 | 326.432 | 58.084 | β | β | β | β |
| Kronberger et al. | 2006 | 326.417 | 58.094 | β | β | β | β |
| Dias et al. | 2002 | 326.433 | 58.084 | β | 1.13 | -2.65 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | β | β | β | β | -0.300* | β | β | β |
| Almeida et al. | 2025 | 5.15 | 2.78 | β | 1442 | β | 975 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1775* | β | β |
| Cavallo et al. | 2024 | 3.80 | 2.89 | β | 1479 | -0.450 | β | β | β |
| Hunt & Reffert | 2023 | 4.19 | 3.29 | 2.06 | 309 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1122 | β | 1084 | β | β |
| Dias et al. | 2021 | 5.15 | 2.78 | β | 1442 | -0.165 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 5.22 | 2.40 | β | 1349 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.05 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 4.05 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.05 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.98 | 2.89 | β | 1122 | β | β | β | β |
| Kharchenko et al. | 2016 | 3.33 | 3.25 | β | 1122 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.33 | 3.25 | β | 1122 | β | β | β | β |
| Kharchenko et al. | 2012 | 3.33 | 3.25 | β | 1122 | β | β | β | β |
| Glushkova et al. | 2010 | 2.65 | 3.26 | β | 1122 | β | β | β | β |
| Dias et al. | 2002 | 2.65 | 3.26 | β | 1122 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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