COIN-Gaia 39
(COIN 39)
0.57
UTI
0.37
CN
0.62
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
3.1 [N/pc2]
- CN 0.37 Poorly populated
- Cdens 0.62 Moderately dense
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 39 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 age and metallicity parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 69.516 | 42.969 | 0.972 | 0.145 | -2.518 | 13.507 |
| Li et al. | 2025 | 69.612 | 42.95 | 0.991 | 0.238 | -2.467 | â |
| Almeida et al. | 2025 | 69.582 | 42.977 | â | â | â | â |
| Zhang et al. | 2024 | 69.581 | 42.97 | â | â | â | â |
| Hunt & Reffert | 2024 | 69.581 | 42.97 | 0.967 | 0.098 | -2.544 | 7.962 |
| Cavallo et al. | 2024 | 69.574 | 42.985 | 0.964 | â | â | â |
| Hunt & Reffert | 2023 | 69.581 | 42.97 | 0.967 | 0.098 | -2.544 | 7.962 |
| He et al. | 2022 | 69.55 | 43.024 | 0.966 | 0.123 | -2.54 | â |
| Dias et al. | 2021 | 69.582 | 42.977 | 0.99 | 0.254 | -2.45 | â |
| Cantat-Gaudin et al. | 2020 | 69.612 | 42.95 | 0.991 | 0.238 | -2.467 | â |
| Cantat-Gaudin & Anders | 2020 | 69.612 | 42.95 | 0.991 | 0.238 | -2.467 | â |
| Monteiro & Dias | 2019 | 69.612 | 42.95 | â | â | â | 2.074 |
| Cantat-Gaudin et al. | 2019 | 69.612 | 42.95 | 0.99 | 0.24 | -2.46 | 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 | 0.99 | 1.25 | 0.44 | 281 | -0.131 | 110 | â | â |
| Li et al. | 2025 | 1.05 | 1.00 | â | 71 | 0.152 | â | â | â |
| Almeida et al. | 2025 | 0.99 | 1.32 | â | 281 | â | 84 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.209(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 137(1) | â | â |
| Cavallo et al. | 2024 | 0.99 | 1.35 | â | 288 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.99 | 0.89 | 0.44 | 274 | â | â | â | â |
| He et al. | 2022 | â | 1.30 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.97 | â | â | 309 | â | â | â | â |
| Dias et al. | 2021 | 0.99 | 1.32 | â | 281 | -0.131 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.01 | 0.63 | â | 288 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.98 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.08 | 1.20 | â | 36 | 0.018 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.98 | 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: good fit.
Cavallo et al. (2024)
Gold sample.