UBC 1267
0.48
UTI
0.32
CN
1.0
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
5.8 [N/pc2]
- CN 0.32 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1267 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large 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 | 72.541 | 43.543 | 0.433 | 0.015 | -1.889 | -15.37 |
| Zhang et al. | 2024 | 72.57 | 43.545 | â | â | â | â |
| Hunt & Reffert | 2024 | 72.57 | 43.545 | 0.438 | 0.012 | -1.888 | -15.571 |
| Cavallo et al. | 2024 | 72.525 | 43.545 | 0.437 | â | â | â |
| Hunt & Reffert | 2023 | 72.57 | 43.545 | 0.438 | 0.012 | -1.888 | -15.571 |
| Castro-Ginard et al. | 2022 | 72.54 | 43.54 | 0.44 | 0.01 | -1.89 | -20.02 |
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 | 2.19 | 0.9 | 0.33 | 502 | -0.108 | 252 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.416(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 252(1) | â | â |
| Cavallo et al. | 2024 | 2.19 | 1.40 | â | 251 | 0.200 | â | â | â |
| Hunt & Reffert | 2023 | 2.12 | 0.90 | 0.33 | 553 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.20 | 0.73 | â | 502 | 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.