Teutsch J1037.3-6034
0.66
UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
1.4 [arcmin]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
Teutsch J1037.3-6034 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.77 kpc) differs significantly from the median photometric distance (~4.13 kpc).
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
Distant
Moderate extinction
Massive
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 | 159.329 | -60.572 | 0.148 | -5.32 | 2.562 | 26.462 |
| Hu & Soubiran | 2025 | 159.327 | -60.572 | â | â | â | â |
| Hunt & Reffert | 2024 | 159.331 | -60.572 | 0.15 | -5.333 | 2.569 | 31.538 |
| Cavallo et al. | 2024 | 159.327 | -60.572 | 0.151 | â | â | â |
| Hunt & Reffert | 2023 | 159.331 | -60.572 | 0.15 | -5.333 | 2.569 | 31.538 |
| Bica et al. | 2019 | 159.337 | -60.574 | 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 | -0.350* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1640* | â | â |
| Cavallo et al. | 2024 | 3.02 | 1.86 | â | 513 | -0.580 | â | â | â |
| Hunt & Reffert | 2023 | 5.24 | 1.41 | 2.20 | 320 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.