UBC 297
0.69
UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 297 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate 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 | 218.074 | -62.206 | 0.344 | -6.774 | -3.955 | -45.972 |
| Hu & Soubiran | 2025 | 218.094 | -62.203 | â | â | â | â |
| Hunt & Reffert | 2024 | 218.062 | -62.212 | 0.351 | -6.793 | -3.972 | -52.957 |
| Cavallo et al. | 2024 | 218.094 | -62.203 | 0.35 | â | â | â |
| Hunt & Reffert | 2023 | 218.062 | -62.212 | 0.351 | -6.793 | -3.972 | -52.957 |
| Cantat-Gaudin et al. | 2020 | 218.081 | -62.222 | 0.327 | -6.779 | -3.923 | â |
| Castro-Ginard et al. | 2020 | 218.133 | -62.211 | 0.327 | -6.786 | -3.919 | 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 | -0.030* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 849* | â | â |
| Cavallo et al. | 2024 | 1.99 | 2.41 | â | 575 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 2.57 | 2.47 | 1.57 | 169 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.72 | 2.11 | â | 355 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.