UBC 1295
0.42
UTI
0.42
CN
0.68
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
6.5 [arcmin]
- CN 0.42 Poorly populated
- Cdens 0.68 Moderately dense
- CC3 0.38 Low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1295 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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
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 | 86.221 | 26.879 | 0.539 | 0.679 | -3.382 | â |
| Zhang et al. | 2024 | 86.217 | 26.896 | â | â | â | â |
| Hunt & Reffert | 2024 | 86.217 | 26.896 | 0.535 | 0.705 | -3.385 | -8.512 |
| Cavallo et al. | 2024 | 86.21 | 26.91 | 0.544 | â | â | â |
| Hunt & Reffert | 2023 | 86.217 | 26.896 | 0.535 | 0.705 | -3.385 | -8.512 |
| Castro-Ginard et al. | 2022 | 86.22 | 26.88 | 0.54 | 0.69 | -3.38 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.047* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 302* | â | â |
| Cavallo et al. | 2024 | 1.78 | 2.02 | â | 219 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.69 | 1.85 | 1.46 | 123 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.09 | 1.71 | â | 150 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.