UBC 260
0.00
UTI
0.3
CN
0.94
Cdens
0.62
CC3
0.38
Clit
0.0
Cdup
Radius (P>50% members)
15.7 [arcmin]
- CN 0.3 Poorly populated
- Cdens 0.94 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.38 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
UBC 260 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, below 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 absorption and age parameters (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 140.04 | -69.981 | 1.806 | -7.712 | 8.04 | 10.673 |
| Li et al. | 2025 | 140.148 | -69.885 | 1.78 | -7.755 | 8.005 | â |
| Alfonso et al. | 2024 | 139.892 | -69.794 | 1.786 | -7.682 | 7.923 | â |
| He et al. | 2022 | 140.082 | -69.896 | 1.831 | -7.676 | 8.062 | â |
| Tarricq et al. | 2022 | 139.668 | -69.881 | 1.816 | -7.697 | 8.009 | â |
| Cantat-Gaudin et al. | 2020 | 140.148 | -69.885 | 1.78 | -7.755 | 8.005 | â |
| Castro-Ginard et al. | 2020 | 140.188 | -69.847 | 1.784 | -7.742 | 8.014 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.55 | 0.25 | â | 299 | -0.060 | â | â | â |
| Alfonso et al. | 2024 | 0.57 | 0.00 | â | 68 | 0.011 | â | â | â |
| He et al. | 2022 | â | 0.25 | â | 63 | â | â | â | â |
| Tarricq et al. | 2022 | 0.56 | â | â | 245 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.57 | 0.00 | â | 234 | â | â | â | â |

