Teutsch 74
(SAI 144; MWSC 3558; DSH J2145.6+5805)
0.79
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.71
Clit
1.0
Cdup
Nm (P>50%)
224
Core radius and density
1.1 [pc], 10 [pc-2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.71 Moderately 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 moderately 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 | 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 |
| Jadhav & Subramaniam | 2021 | 326.422 | 58.097 | 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 |
| Sampedro et al. | 2017 | 326.433 | 58.084 | β | 1.5 | -3.21 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 4.05 | 3.115 | 2.06 | 1122 | -0.300 | 1430 | β | 3 |
| Hu & Soubiran | 2025 | β | β | β | β | -0.300(5) | β | β | β |
| Almeida et al. | 2025 | 5.15 | 2.78 | β | 1442 | β | 975 | β | β |
| Hunt & Reffert | 2024 | 4.19 | 3.29 | 2.06 | 309 | β | 1775(1) | 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 |
| Jadhav & Subramaniam | 2021 | 5.22 | 2.40 | β | 1349 | β | 2886 | β | 3(1) |
| 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 |
| Kounkel et al. | 2020 | 3.90 | 2.73 | β | 1148 | 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 | 2.94 | β | 1122 | β | β | β | β |
| Kharchenko et al. | 2016 | 3.33 | 3.31 | β | 1122 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.33 | 3.31 | β | 1122 | β | β | β | β |
| Kharchenko et al. | 2012 | 3.33 | 3.31 | β | 1122 | β | β | β | β |
| Glushkova et al. | 2010 | 2.65 | 3.31 | β | 1122 | β | β | β | β |
| Dias et al. | 2002 | 2.65 | 3.31 | β | 1122 | 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: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.41 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.41 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1048, e_all=0.1251.
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.