Teutsch 127
0.78
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
11.4 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 127 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. 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 | 334.746 | 56.101 | 0.236 | -3.365 | -2.514 | -60.771 |
| Almeida et al. | 2025 | 334.747 | 56.113 | â | â | â | â |
| Hunt & Reffert | 2024 | 334.743 | 56.123 | 0.235 | -3.336 | -2.529 | â |
| Celli et al. | 2024 | 334.747 | 56.124 | â | â | â | â |
| Cavallo et al. | 2024 | 334.736 | 56.109 | 0.235 | â | â | â |
| Hunt & Reffert | 2023 | 334.743 | 56.123 | 0.235 | -3.336 | -2.529 | â |
| Dias et al. | 2021 | 334.747 | 56.113 | 0.235 | -3.331 | -2.423 | â |
| Cantat-Gaudin et al. | 2020 | 334.747 | 56.121 | 0.242 | -3.344 | -2.417 | â |
| Cantat-Gaudin & Anders | 2020 | 334.747 | 56.121 | 0.242 | -3.344 | -2.417 | â |
| Cantat-Gaudin et al. | 2018 | 334.747 | 56.121 | 0.242 | -3.344 | -2.417 | â |
| Dias et al. | 2014 | 334.75 | 56.124 | â | -2.09 | -2.0 | â |
| Kronberger et al. | 2006 | 334.747 | 56.124 | â | â | â | â |
| Dias et al. | 2002 | 334.75 | 56.124 | 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 | 3.69 | 2.29 | 1.28 | 8 | 0.543 | 353 | â | â |
| Liu et al. | 2025 | 4.39 | 0.75 | â | 13 | â | â | â | â |
| Almeida et al. | 2025 | 3.79 | 2.29 | â | 6 | â | 313 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 491(1) | â | â |
| Celli et al. | 2024 | â | â | â | 12 | â | 353 | â | â |
| Cavallo et al. | 2024 | 2.59 | 0.99 | â | 23 | 1.240 | â | â | â |
| Hunt & Reffert | 2023 | 4.21 | 2.45 | 1.28 | 3 | â | â | â | â |
| Dias et al. | 2021 | 3.79 | 2.29 | â | 6 | -0.154 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.45 | 2.08 | â | 11 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.69 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.69 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 3.60 | 18.26 | â | 5 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 175 along with HSC_797.
Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P528, along with HSC_797.
Cavallo et al. (2024)
Bronze sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.