UBC 618
0.63
UTI
0.33
CN
0.97
Cdens
1.0
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
1.4 [arcmin]
- CN 0.33 Poorly populated
- Cdens 0.97 Very dense
- CC3 1.0 Very high quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 618 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large 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.
Very distant
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 | 96.24 | 7.601 | 0.156 | 0.236 | 0.044 | 38.027 |
| Almeida et al. | 2025 | 96.259 | 7.612 | â | â | â | â |
| Hunt & Reffert | 2024 | 96.238 | 7.618 | 0.14 | 0.224 | 0.039 | 38.028 |
| Cavallo et al. | 2024 | 96.249 | 7.6 | 0.136 | â | â | â |
| Hunt & Reffert | 2023 | 96.238 | 7.618 | 0.14 | 0.224 | 0.039 | 38.028 |
| Dias et al. | 2021 | 96.259 | 7.612 | 0.144 | 0.25 | 0.018 | 37.319 |
| Cantat-Gaudin et al. | 2020 | 96.241 | 7.617 | 0.132 | 0.251 | 0.062 | â |
| Castro-Ginard et al. | 2020 | 96.259 | 7.618 | 0.133 | 0.235 | 0.051 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 5.39 | 1.55 | â | 358 | â | 484 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 513* | â | â |
| Cavallo et al. | 2024 | 4.85 | 1.81 | â | 219 | -0.440 | â | â | â |
| Hunt & Reffert | 2023 | 6.80 | 1.48 | 0.68 | 268 | â | â | â | â |
| Dias et al. | 2021 | 5.39 | 1.55 | â | 358 | -0.104 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.01 | 0.90 | â | 724 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.