UBC 1254
0.63
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
5.4 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1254 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, 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 moderate percentage of members with 3 later reported entries. See table with shared members information.
Relatively close
High extinction
Massive
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 | 56.334 | 50.734 | 0.341 | 0.796 | -1.251 | -43.296 |
| Zhang et al. | 2024 | 56.309 | 50.752 | â | â | â | â |
| Hunt & Reffert | 2024 | 56.309 | 50.752 | 0.344 | 0.789 | -1.25 | -9.928 |
| Cavallo et al. | 2024 | 56.342 | 50.724 | 0.343 | â | â | â |
| Hunt & Reffert | 2023 | 56.309 | 50.752 | 0.344 | 0.789 | -1.25 | -9.928 |
| Castro-Ginard et al. | 2022 | 56.34 | 50.73 | 0.34 | 0.8 | -1.25 | -17.48 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.070* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1079* | â | â |
| Cavallo et al. | 2024 | 2.63 | 3.32 | â | 490 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 2.65 | 3.27 | 1.92 | 186 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 3.15 | 2.45 | â | 489 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.