UBC 295
0.68
UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
5.6 [arcmin]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 295 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low 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 moderate 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 | 207.572 | -60.399 | 0.583 | -4.539 | -1.508 | -10.993 |
| Li et al. | 2025 | 207.554 | -60.399 | 0.578 | -4.487 | -1.54 | â |
| Hunt & Reffert | 2024 | 207.586 | -60.41 | 0.579 | -4.552 | -1.504 | -15.433 |
| Cavallo et al. | 2024 | 207.553 | -60.391 | 0.579 | â | â | â |
| Hunt & Reffert | 2023 | 207.586 | -60.41 | 0.579 | -4.552 | -1.504 | -15.433 |
| Cantat-Gaudin et al. | 2020 | 207.554 | -60.399 | 0.578 | -4.487 | -1.54 | â |
| Castro-Ginard et al. | 2020 | 207.537 | -60.409 | 0.579 | -4.486 | -1.54 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.51 | 0.71 | â | 676 | 0.172 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 335* | â | â |
| Cavallo et al. | 2024 | 1.40 | 1.03 | â | 490 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 1.61 | 0.95 | 0.41 | 312 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.72 | 0.95 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.