Teutsch 187
0.32
UTI
0.37
CN
0.3
Cdens
0.75
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
37
Core radius and density
1.7 [pc], 1.5 [pc-2]
- CN 0.37 Poorly populated
- Cdens 0.3 Loose
- CC3 0.75 High quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Teutsch 187 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later 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 | 19.699 | 59.442 | 0.145 | -1.426 | 0.395 | â |
| Hu & Soubiran | 2025 | 19.72 | 59.438 | â | â | â | â |
| Hunt & Reffert | 2024 | 19.696 | 59.441 | 0.144 | -1.425 | 0.388 | â |
| Cavallo et al. | 2024 | 19.719 | 59.438 | 0.14 | â | â | â |
| Hunt & Reffert | 2023 | 19.696 | 59.441 | 0.144 | -1.425 | 0.388 | â |
| Bica et al. | 2019 | 19.703 | 59.447 | 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 | 6.39 | 1.93 | 1.67 | 706 | -0.215 | 443 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.150(5) | â | â | â |
| Hunt & Reffert | 2024 | 6.39 | 1.93 | 1.67 | 706 | â | 443(1) | â | â |
| Cavallo et al. | 2024 | 4.17 | 1.77 | â | 1738 | -0.280 | â | â | â |
| Hunt & Reffert | 2023 | 6.39 | 1.93 | 1.67 | 706 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.87 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.87 (50th percentile).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.