Teutsch 143b
(DSH J1108.5-6044)
0.08
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.35
Clit
0.11
Cdup
Stellar density (N50/rad)
31.9 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 0.11 Likely duplicate
Overview
Teutsch 143b 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 moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 167.15 | -60.739 | 0.221 | -5.623 | 2.268 | 20.097 |
| Hu & Soubiran | 2025 | 167.144 | -60.742 | â | â | â | â |
| Hunt & Reffert | 2024 | 167.146 | -60.745 | 0.221 | -5.628 | 2.277 | 19.624 |
| Cavallo et al. | 2024 | 167.144 | -60.742 | 0.223 | â | â | â |
| Hunt & Reffert | 2023 | 167.146 | -60.745 | 0.221 | -5.628 | 2.277 | 19.624 |
| Bica et al. | 2019 | 167.147 | -60.744 | â | â | â | â |
| Kronberger et al. | 2006 | 167.128 | -60.747 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.595 | 2.12 | 1.77 | 674 | -0.080 | 1479 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.290(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1479(1) | â | â |
| Cavallo et al. | 2024 | 3.12 | 2.02 | â | 977 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 4.07 | 2.22 | 1.77 | 370 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.