UBC 407
0.39
UTI
0.25
CN
0.26
Cdens
0.62
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
1.3 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 0.26 Loose
- CC3 0.62 Intermediate quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 407 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 4.576 | 63.383 | 0.307 | -3.113 | -0.594 | â |
| Almeida et al. | 2025 | 4.553 | 63.345 | â | â | â | â |
| Hunt & Reffert | 2024 | 4.636 | 63.366 | 0.292 | -3.12 | -0.629 | â |
| Cavallo et al. | 2024 | 4.537 | 63.379 | 0.294 | â | â | â |
| Hunt & Reffert | 2023 | 4.636 | 63.366 | 0.292 | -3.12 | -0.629 | â |
| Dias et al. | 2021 | 4.553 | 63.345 | 0.289 | -3.084 | -0.57 | -75.435 |
| Cantat-Gaudin et al. | 2020 | 4.566 | 63.367 | 0.302 | -3.085 | -0.537 | â |
| Castro-Ginard et al. | 2020 | 4.554 | 63.347 | 0.303 | -3.092 | -0.545 | 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 | 3.05 | 1.68 | 2.03 | 66 | 0.209 | 1198 | â | â |
| Almeida et al. | 2025 | 2.78 | 1.68 | â | 66 | â | 1964 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 431(1) | â | â |
| Cavallo et al. | 2024 | 3.60 | 1.81 | â | 21 | 0.420 | â | â | â |
| Hunt & Reffert | 2023 | 3.05 | 1.61 | 2.03 | 102 | â | â | â | â |
| Dias et al. | 2021 | 2.78 | 1.68 | â | 66 | -0.001 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.31 | 1.38 | â | 38 | 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.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.