UBC 10 a
0.44
UTI
0.0
CN
0.21
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
1.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.21 Very loose
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 10 a is a sparse, very loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately 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 | 324.518 | 62.1 | 1.084 | -2.115 | -3.154 | -19.138 |
| Li et al. | 2025 | 324.652 | 62.206 | 1.075 | -2.131 | -3.031 | â |
| Alfonso et al. | 2024 | 325.041 | 62.305 | 1.012 | -2.663 | -3.147 | â |
| Hunt & Reffert | 2024 | 325.278 | 61.968 | 1.115 | -3.32 | -4.831 | -6.086 |
| Celli et al. | 2024 | 324.652 | 62.206 | â | â | â | â |
| Cavallo et al. | 2024 | 325.587 | 62.29 | 1.117 | â | â | â |
| Hunt & Reffert | 2023 | 325.278 | 61.968 | 1.115 | -3.32 | -4.831 | -6.086 |
| He et al. | 2022 | 324.804 | 62.357 | 1.086 | -2.043 | -3.107 | â |
| Cantat-Gaudin et al. | 2020 | 324.652 | 62.206 | 1.075 | -2.131 | -3.031 | â |
| Cantat-Gaudin & Anders | 2020 | 324.652 | 62.206 | 1.075 | -2.131 | -3.031 | â |
| Bica et al. | 2019 | 324.426 | 61.753 | â | â | â | â |
| Castro-Ginard et al. | 2018 | 324.439 | 61.76 | 1.079 | -2.147 | -3.035 | -23.12 |
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 | 0.87 | 1.19 | 0.56 | 15 | 0.010 | 126 | â | â |
| Li et al. | 2025 | 0.78 | 1.26 | â | 15 | -0.130 | â | â | â |
| Alfonso et al. | 2024 | 0.87 | 0.89 | â | 63 | 0.010 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 48(1) | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 205 | â | â |
| Cavallo et al. | 2024 | 0.97 | 1.31 | â | 30 | 0.380 | â | â | â |
| Hunt & Reffert | 2023 | 0.85 | 1.12 | 0.56 | 45 | â | â | â | â |
| He et al. | 2022 | â | 1.30 | â | 11 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.87 | 0.89 | â | 14 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.91 | â | â | â | 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.