UBC 1313
0.53
UTI
0.6
CN
0.61
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
3.1 [N/pc2]
- CN 0.6 Moderately populated
- Cdens 0.61 Moderately dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1313 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a large 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 metallicity parameter (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 | 96.897 | 17.191 | 0.187 | 0.687 | 0.013 | 22.693 |
| Hu & Soubiran | 2025 | 96.901 | 17.177 | â | â | â | â |
| Zhang et al. | 2024 | 96.892 | 17.189 | â | â | â | â |
| Hunt & Reffert | 2024 | 96.892 | 17.189 | 0.184 | 0.709 | -0.002 | 19.562 |
| Cavallo et al. | 2024 | 96.901 | 17.177 | 0.187 | â | â | â |
| Hunt & Reffert | 2023 | 96.892 | 17.189 | 0.184 | 0.709 | -0.002 | 19.562 |
| Castro-Ginard et al. | 2022 | 96.9 | 17.19 | 0.2 | 0.71 | 0.02 | 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 | 4.57 | 1.35 | 2.15 | 661 | -0.250 | 708 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.250(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.341(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 708(1) | â | â |
| Cavallo et al. | 2024 | 3.42 | 1.42 | â | 661 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 4.57 | 1.35 | 2.15 | 378 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 4.69 | 0.86 | â | 1094 | 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.