UPK 621
0.74
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
10.0 [arcmin]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 621 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near 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 age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
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 | 237.129 | -54.428 | 1.113 | -2.498 | -3.122 | -1.099 |
| Li et al. | 2025 | 237.093 | -54.403 | 1.122 | -2.48 | -3.105 | â |
| Almeida et al. | 2025 | 237.199 | -54.385 | â | â | â | â |
| Alfonso et al. | 2024 | 237.019 | -54.401 | 1.076 | -2.556 | -3.086 | â |
| Hunt & Reffert | 2024 | 237.201 | -54.415 | 1.102 | -2.471 | -3.084 | -4.385 |
| Celli et al. | 2024 | 237.093 | -54.403 | â | â | â | â |
| Cavallo et al. | 2024 | 237.225 | -54.431 | 1.106 | â | â | â |
| Hunt & Reffert | 2023 | 237.201 | -54.415 | 1.102 | -2.471 | -3.084 | -4.385 |
| Almeida et al. | 2023 | 237.425 | -54.511 | â | â | â | â |
| Dias et al. | 2021 | 237.199 | -54.385 | 1.126 | -2.471 | -3.101 | â |
| Cantat-Gaudin et al. | 2020 | 237.093 | -54.403 | 1.122 | -2.48 | -3.105 | â |
| Cantat-Gaudin & Anders | 2020 | 237.087 | -54.417 | 1.111 | -2.485 | -3.093 | â |
| Sim et al. | 2019 | 237.205 | -54.419 | â | -2.57 | -3.08 | 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 | 0.85 | 0.83 | â | 80 | -0.040 | â | â | â |
| Almeida et al. | 2025 | 0.88 | 0.94 | â | 36 | â | 91 | â | â |
| Alfonso et al. | 2024 | 0.84 | 0.66 | â | 48 | 0.150 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 127* | â | â |
| Celli et al. | 2024 | â | â | â | 26 | â | 150 | â | â |
| Cavallo et al. | 2024 | 0.92 | 1.02 | â | 18 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.87 | 0.90 | 1.08 | 65 | â | â | â | â |
| Almeida et al. | 2023 | 0.87 | 1.10 | â | 149 | 0.019 | 488* | 0.68 | â |
| Dias et al. | 2021 | 0.88 | 0.94 | â | 36 | 0.150 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.84 | 0.66 | â | 26 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.88 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.87 | â | â | 631 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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