UPK 113
0.75
UTI
0.59
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
14.2 [arcmin]
- CN 0.59 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 113 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 317.49 | 34.248 | 1.422 | 2.164 | -2.365 | -14.749 |
| Li et al. | 2025 | 317.505 | 34.347 | 1.434 | 2.169 | -2.418 | â |
| Almeida et al. | 2025 | 317.443 | 34.377 | â | â | â | â |
| Alfonso et al. | 2024 | 317.477 | 34.405 | 1.39 | 2.167 | -2.357 | â |
| Hunt & Reffert | 2024 | 317.527 | 34.278 | 1.426 | 2.121 | -2.402 | -9.845 |
| Cavallo et al. | 2024 | 317.394 | 34.398 | 1.423 | â | â | â |
| Hunt & Reffert | 2023 | 317.527 | 34.278 | 1.426 | 2.121 | -2.402 | -9.845 |
| He et al. | 2022 | 317.467 | 34.234 | 1.424 | 2.202 | -2.39 | â |
| Dias et al. | 2021 | 317.443 | 34.377 | 1.415 | 2.193 | -2.415 | -14.576 |
| Cantat-Gaudin et al. | 2020 | 317.505 | 34.347 | 1.434 | 2.169 | -2.418 | â |
| Cantat-Gaudin & Anders | 2020 | 317.509 | 34.347 | 1.425 | 2.187 | -2.498 | â |
| Sim et al. | 2019 | 317.451 | 34.364 | â | 2.16 | -2.34 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.59 | 0.28 | â | 64 | -0.252 | â | â | â |
| Almeida et al. | 2025 | 0.68 | 0.31 | â | 64 | â | 70 | â | â |
| Alfonso et al. | 2024 | 0.72 | 0.15 | â | 42 | 0.030 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 89* | â | â |
| Cavallo et al. | 2024 | 0.71 | 0.18 | â | 39 | 0.380 | â | â | â |
| Hunt & Reffert | 2023 | 0.67 | 0.13 | 0.52 | 48 | â | â | â | â |
| He et al. | 2022 | â | 0.35 | â | 35 | â | â | â | â |
| Tarricq et al. | 2022 | 0.70 | â | â | 52 | â | â | â | â |
| Dias et al. | 2021 | 0.68 | 0.31 | â | 64 | 0.030 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.72 | 0.15 | â | 49 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.69 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.68 | â | â | 71 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.