UBC 1455
0.40
UTI
0.34
CN
0.4
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
9.9 [arcmin]
- CN 0.34 Poorly populated
- Cdens 0.4 Loose
- CC3 0.62 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1455 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively 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 metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively 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 | 131.112 | -54.138 | 0.701 | -3.501 | 6.602 | 28.661 |
| Hu & Soubiran | 2025 | 131.694 | -54.638 | â | â | â | â |
| Hunt & Reffert | 2024 | 131.002 | -54.129 | 0.703 | -3.535 | 6.636 | 28.596 |
| Cavallo et al. | 2024 | 131.694 | -54.638 | 0.708 | â | â | â |
| Hunt & Reffert | 2023 | 131.002 | -54.129 | 0.703 | -3.535 | 6.636 | 28.596 |
| Castro-Ginard et al. | 2022 | 131.13 | -54.13 | 0.7 | -3.49 | 6.6 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.120* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 140* | â | â |
| Cavallo et al. | 2024 | 1.68 | 0.57 | â | 676 | 0.880 | â | â | â |
| Hunt & Reffert | 2023 | 1.35 | 0.33 | 0.92 | 738 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 1.45 | 0.62 | â | 410 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.