UBC 270
0.66
UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
15.8 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 270 is a moderately populated, very dense object of high 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, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately 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 | 169.821 | -59.561 | 0.4 | -6.348 | 1.153 | â |
| Li et al. | 2025 | 169.813 | -59.552 | 0.389 | -6.333 | 1.122 | â |
| Almeida et al. | 2025 | 169.787 | -59.548 | â | â | â | â |
| Hunt & Reffert | 2024 | 169.828 | -59.569 | 0.404 | -6.334 | 1.171 | â |
| Cavallo et al. | 2024 | 169.802 | -59.561 | 0.404 | â | â | â |
| Hunt & Reffert | 2023 | 169.828 | -59.569 | 0.404 | -6.334 | 1.171 | â |
| Almeida et al. | 2023 | 169.805 | -59.553 | â | â | â | â |
| Dias et al. | 2021 | 169.787 | -59.548 | 0.395 | -6.365 | 1.133 | â |
| Cantat-Gaudin et al. | 2020 | 169.813 | -59.552 | 0.389 | -6.333 | 1.122 | â |
| Castro-Ginard et al. | 2020 | 169.789 | -59.544 | 0.394 | -6.35 | 1.13 | 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 | 2.36 | 1.1 | 1.32 | 38 | 0.072 | 425 | 0.61 | â |
| Li et al. | 2025 | 2.36 | 0.98 | â | 153 | 0.068 | â | â | â |
| Almeida et al. | 2025 | 2.41 | 1.25 | â | 13 | â | 213 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 425(1) | â | â |
| Cavallo et al. | 2024 | 2.31 | 1.10 | â | 38 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 2.24 | 0.92 | 1.32 | 33 | â | â | â | â |
| Almeida et al. | 2023 | 2.23 | 1.21 | â | 81 | 0.076 | 758(1) | 0.61 | â |
| Dias et al. | 2021 | 2.41 | 1.25 | â | 13 | 0.048 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.55 | 0.67 | â | 162 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P470, along with HSC_2427.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.