Teutsch J1037.3-6034
0.52
UTI
0.66
CN
0.75
Cdens
1.0
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
81
Core radius and density
1.4 [pc], 3.7 [pc-2]
- CN 0.66 Moderately populated
- Cdens 0.75 Dense
- CC3 1.0 Very high quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Teutsch J1037.3-6034 is a moderately populated, 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 rarely studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. 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 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 5.24 | 1.41 | 2.2 | 320 | -0.465 | 1640 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.350(5) | â | â | â |
| Hunt & Reffert | 2024 | 5.24 | 1.41 | 2.20 | 320 | â | 1640(1) | 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 |
(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: 0.91 (50th percentile).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.