Teutsch 80
(MWSC 2258; DSH J1453.4-6028)
0.90
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
2.0 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Teutsch 80 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Relatively close
High extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 223.357 | -60.477 | 0.346 | -5.582 | -3.646 | -22.539 |
| Almeida et al. | 2025 | 223.367 | -60.485 | â | â | â | â |
| Hunt & Reffert | 2024 | 223.359 | -60.474 | 0.339 | -5.586 | -3.678 | -14.6 |
| Cavallo et al. | 2024 | 223.365 | -60.482 | 0.345 | â | â | â |
| Hunt & Reffert | 2023 | 223.359 | -60.474 | 0.339 | -5.586 | -3.678 | -14.6 |
| Just et al. | 2023 | 223.338 | -60.483 | â | â | â | â |
| Dias et al. | 2021 | 223.367 | -60.485 | 0.34 | -5.543 | -3.603 | -23.539 |
| Cantat-Gaudin et al. | 2020 | 223.361 | -60.478 | 0.349 | -5.553 | -3.581 | â |
| Cantat-Gaudin & Anders | 2020 | 223.361 | -60.478 | 0.349 | -5.553 | -3.581 | â |
| Soubiran et al. | 2018 | 223.361 | -60.478 | â | â | â | -23.48 |
| Bica et al. | 2019 | 223.369 | -60.482 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 223.361 | -60.478 | 0.349 | -5.553 | -3.581 | â |
| Kharchenko et al. | 2016 | 223.338 | -60.483 | â | â | â | â |
| Dias et al. | 2014 | 223.358 | -60.483 | â | -1.94 | -1.89 | â |
| Kharchenko et al. | 2013 | 223.35 | -60.485 | â | -6.78 | 0.42 | â |
| Kronberger et al. | 2006 | 223.357 | -60.483 | â | â | â | â |
| Dias et al. | 2002 | 223.358 | -60.483 | â | -1.94 | -1.89 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.16 | 3.85 | â | 635 | â | 841 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2258* | â | â |
| Cavallo et al. | 2024 | 2.55 | 5.01 | â | 186 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 2.64 | 5.15 | 2.79 | 92 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 56 | â | 492 | â | â |
| Dias et al. | 2021 | 2.16 | 3.85 | â | 635 | 0.228 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.43 | 4.00 | â | 224 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.65 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.65 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.35 | 5.23 | â | 56 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.35 | 5.23 | â | 56 | â | â | â | â |
| Kronberger et al. | 2006 | 2.50* | 4.99* | â | 126* | â | â | â | â |
| Dias et al. | 2002 | 2.50 | 4.99 | â | 126 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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