UPK 398
(OCSN 308)
0.85
UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
15.5 [arcmin]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
UPK 398 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is well-studied in the literature.
Very close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 86.019 | 7.035 | 2.24 | -3.26 | -1.781 | 29.613 |
| Li et al. | 2025 | 85.994 | 7.021 | 2.176 | -3.315 | -1.714 | â |
| Almeida et al. | 2025 | 85.989 | 7.063 | â | â | â | â |
| Alfonso et al. | 2024 | 85.995 | 7.024 | 2.2 | -3.213 | -1.777 | â |
| Zhang et al. | 2024 | 85.956 | 7.059 | â | â | â | â |
| Hunt & Reffert | 2024 | 85.956 | 7.059 | 2.251 | -3.257 | -1.748 | 25.231 |
| Celli et al. | 2024 | 85.994 | 7.021 | â | â | â | â |
| Cavallo et al. | 2024 | 86.093 | 7.006 | 2.255 | â | â | â |
| Hunt & Reffert | 2023 | 85.956 | 7.059 | 2.251 | -3.257 | -1.748 | 25.231 |
| Qin et al. | 2023 | 85.96 | 7.04 | 2.26 | -3.27 | -1.74 | 27.92 |
| He et al. | 2022 | 86.057 | 7.039 | 2.26 | -3.232 | -1.761 | â |
| Dias et al. | 2021 | 85.989 | 7.063 | 2.172 | -3.298 | -1.747 | 30.658 |
| Cantat-Gaudin et al. | 2020 | 85.994 | 7.021 | 2.176 | -3.315 | -1.714 | â |
| Cantat-Gaudin & Anders | 2020 | 85.984 | 7.02 | 2.196 | -3.276 | -1.737 | â |
| Sim et al. | 2019 | 86.012 | 7.027 | â | -3.34 | -1.76 | 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 | 0.49 | 0.45 | â | 5 | -0.174 | â | â | â |
| Almeida et al. | 2025 | 0.45 | 0.47 | â | 14 | â | 65 | â | â |
| Alfonso et al. | 2024 | 0.45 | 0.38 | â | 11 | 0.007 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.059* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 51* | â | â |
| Celli et al. | 2024 | â | â | â | 11 | â | 57 | â | â |
| Cavallo et al. | 2024 | 0.49 | 1.00 | â | 4 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.43 | 0.80 | 1.03 | 12 | â | â | â | â |
| Qin et al. | 2023 | 0.50 | 0.31 | â | 7 | â | â | â | â |
| He et al. | 2022 | â | 0.05 | â | 9 | â | â | â | â |
| Dias et al. | 2021 | 0.45 | 0.47 | â | 14 | 0.007 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.45 | 0.38 | â | 11 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.45 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.45 | â | â | 13 | 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.