UPK 613
0.63
UTI
0.34
CN
0.75
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Stellar density (N50/rad)
3.8 [N/pc2]
- CN 0.34 Poorly populated
- Cdens 0.75 Dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 613 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 226.296 | -49.152 | 1.134 | -4.503 | -3.635 | -27.133 |
| Li et al. | 2025 | 226.276 | -49.152 | 1.146 | -4.566 | -3.64 | â |
| Almeida et al. | 2025 | 226.226 | -49.151 | â | â | â | â |
| Alfonso et al. | 2024 | 226.232 | -49.12 | 1.076 | -4.499 | -3.676 | â |
| Hunt & Reffert | 2024 | 226.289 | -49.162 | 1.12 | -4.439 | -3.676 | -29.78 |
| Cavallo et al. | 2024 | 226.294 | -49.121 | 1.127 | â | â | â |
| Hunt & Reffert | 2023 | 226.289 | -49.162 | 1.12 | -4.439 | -3.676 | -29.78 |
| Almeida et al. | 2023 | 226.26 | -49.144 | â | â | â | â |
| Dias et al. | 2021 | 226.226 | -49.151 | 1.149 | -4.556 | -3.672 | â |
| Cantat-Gaudin et al. | 2020 | 226.276 | -49.152 | 1.146 | -4.566 | -3.64 | â |
| Cantat-Gaudin & Anders | 2020 | 226.309 | -49.152 | 1.13 | -4.536 | -3.682 | â |
| Sim et al. | 2019 | 226.221 | -49.164 | â | -4.54 | -3.63 | 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 | 0.84 | 0.565 | 0.48 | 136 | -0.231 | 101 | 0.72 | â |
| Li et al. | 2025 | 0.79 | 0.55 | â | 239 | -0.357 | â | â | â |
| Almeida et al. | 2025 | 0.84 | 0.58 | â | 136 | â | 101 | â | â |
| Alfonso et al. | 2024 | 0.85 | 0.28 | â | 83 | -0.033 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 63(1) | â | â |
| Cavallo et al. | 2024 | 0.81 | 0.66 | â | 251 | -0.590 | â | â | â |
| Hunt & Reffert | 2023 | 0.84 | 0.36 | 0.48 | 213 | â | â | â | â |
| Almeida et al. | 2023 | 0.84 | 0.66 | â | 244 | -0.231 | 117(1) | 0.72 | â |
| Tarricq et al. | 2022 | 0.84 | â | â | 85 | â | â | â | â |
| Dias et al. | 2021 | 0.84 | 0.58 | â | 136 | -0.034 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.86 | 0.28 | â | 83 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.86 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.87 | â | â | 71 | 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.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.