Teutsch 20
(DSH J0628.8+1455)
0.68
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
Teutsch 20 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
Moderate 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 | 97.201 | 14.917 | 0.348 | 1.239 | -1.371 | 49.323 |
| Hu & Soubiran | 2025 | 97.192 | 14.922 | â | â | â | â |
| Zhang et al. | 2024 | 97.202 | 14.921 | â | â | â | â |
| Hunt & Reffert | 2024 | 97.202 | 14.921 | 0.343 | 1.221 | -1.364 | 38.982 |
| Cavallo et al. | 2024 | 97.192 | 14.922 | 0.347 | â | â | â |
| Hunt & Reffert | 2023 | 97.202 | 14.921 | 0.343 | 1.221 | -1.364 | 38.982 |
| Bica et al. | 2019 | 97.205 | 14.916 | â | â | â | â |
| Kronberger et al. | 2006 | 97.206 | 14.921 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.120* | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.226* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 654* | â | â |
| Cavallo et al. | 2024 | 2.75 | 1.63 | â | 759 | -0.190 | â | â | â |
| Hunt & Reffert | 2023 | 2.56 | 1.17 | 1.24 | 551 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.