COIN-Gaia 32
(COIN 32)
0.63
UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
5.1 [N/pc2]
- CN 0.29 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 32 is a poorly populated, very 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 age and metallicity parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 28.2 | 63.053 | 0.793 | 0.005 | -2.306 | -49.725 |
| Li et al. | 2025 | 28.194 | 63.066 | 0.775 | 0.053 | -2.195 | â |
| Almeida et al. | 2025 | 28.165 | 63.06 | â | â | â | â |
| Hunt & Reffert | 2024 | 28.119 | 63.101 | 0.787 | 0.009 | -2.323 | -51.514 |
| Cavallo et al. | 2024 | 28.161 | 63.042 | 0.789 | â | â | â |
| Hunt & Reffert | 2023 | 28.119 | 63.101 | 0.787 | 0.009 | -2.323 | -51.514 |
| Almeida et al. | 2023 | 28.209 | 63.039 | â | â | â | â |
| He et al. | 2022 | 28.188 | 63.053 | 0.793 | -0.001 | -2.306 | â |
| Tarricq et al. | 2022 | 28.187 | 63.079 | 0.793 | -0.009 | -2.299 | â |
| Dias et al. | 2021 | 28.165 | 63.06 | 0.77 | 0.042 | -2.202 | â |
| Cantat-Gaudin et al. | 2020 | 28.194 | 63.066 | 0.775 | 0.053 | -2.195 | â |
| Cantat-Gaudin & Anders | 2020 | 28.194 | 63.066 | 0.775 | 0.053 | -2.195 | â |
| Monteiro & Dias | 2019 | 28.194 | 63.066 | â | â | â | 2.616 |
| Cantat-Gaudin et al. | 2019 | 28.194 | 63.066 | 0.78 | 0.05 | -2.2 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.21 | 1.44 | 0.61 | 217 | -0.026 | 109 | 0.7 | â |
| Li et al. | 2025 | 1.11 | 1.42 | â | 532 | -0.144 | â | â | â |
| Almeida et al. | 2025 | 1.19 | 1.65 | â | 217 | â | 103 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 109(1) | â | â |
| Cavallo et al. | 2024 | 1.30 | 1.44 | â | 355 | 0.580 | â | â | â |
| Hunt & Reffert | 2023 | 1.21 | 1.43 | 0.61 | 121 | â | â | â | â |
| Almeida et al. | 2023 | 1.21 | 1.67 | â | 163 | -0.121 | 114(1) | 0.70 | â |
| He et al. | 2022 | â | 1.95 | â | 32 | â | â | â | â |
| Tarricq et al. | 2022 | 1.20 | â | â | 389 | â | â | â | â |
| Dias et al. | 2021 | 1.19 | 1.65 | â | 217 | -0.026 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.25 | 0.82 | â | 363 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.24 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.34 | 1.19 | â | 175 | 0.032 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 1.25 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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