UBC 1611
0.41
UTI
0.25
CN
0.96
Cdens
0.25
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
4.8 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 0.96 Very dense
- CC3 0.25 Low quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1611 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above 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 age and metallicity parameters (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 | 95.993 | 20.509 | 0.446 | 0.138 | -1.344 | 42.298 |
| Zhang et al. | 2024 | 95.991 | 20.507 | â | â | â | â |
| Hunt & Reffert | 2024 | 95.991 | 20.507 | 0.445 | 0.125 | -1.353 | 42.293 |
| Cavallo et al. | 2024 | 95.984 | 20.505 | 0.446 | â | â | â |
| Hunt & Reffert | 2023 | 95.991 | 20.507 | 0.445 | 0.125 | -1.353 | 42.293 |
| Castro-Ginard et al. | 2022 | 95.98 | 20.5 | 0.44 | 0.14 | -1.34 | 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 | 2.2 | 1.5 | 1.35 | 240 | 0.198 | 134 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.194(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 134(1) | â | â |
| Cavallo et al. | 2024 | 2.20 | 1.59 | â | 240 | 0.590 | â | â | â |
| Hunt & Reffert | 2023 | 2.05 | 1.10 | 1.35 | 495 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.53 | 1.50 | â | 107 | 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.