UBC 419
0.31
UTI
0.0
CN
0.11
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.11 Very loose
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 419 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is poorly studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. 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 | 34.605 | 58.981 | 0.4 | -0.922 | -0.66 | â |
| Li et al. | 2025 | 34.694 | 58.924 | 0.395 | -0.921 | -0.586 | â |
| Hunt & Reffert | 2024 | 34.891 | 58.883 | 0.402 | -0.861 | -0.691 | -54.157 |
| Cavallo et al. | 2024 | 34.764 | 59.032 | 0.402 | â | â | â |
| Hunt & Reffert | 2023 | 34.891 | 58.883 | 0.402 | -0.861 | -0.691 | -54.157 |
| Cantat-Gaudin et al. | 2020 | 34.694 | 58.924 | 0.395 | -0.921 | -0.586 | â |
| Castro-Ginard et al. | 2020 | 34.692 | 58.931 | 0.396 | -0.908 | -0.594 | 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 | 2.315 | 1.595 | 2.42 | 136 | 0.268 | 445 | â | â |
| Li et al. | 2025 | 1.02 | 0.24 | â | 2018 | -0.165 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 445(1) | â | â |
| Cavallo et al. | 2024 | 2.74 | 1.97 | â | 72 | 0.700 | â | â | â |
| Hunt & Reffert | 2023 | 2.29 | 2.04 | 2.42 | 61 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.34 | 1.22 | â | 200 | 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.