COIN-Gaia 40
(COIN 40)
0.72
UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
7.8 [N/pc2]
- CN 0.58 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 40 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 moderately 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 | 81.897 | 33.522 | 0.471 | 0.338 | -2.79 | 54.239 |
| Li et al. | 2025 | 81.874 | 33.526 | 0.47 | 0.393 | -2.762 | â |
| Almeida et al. | 2025 | 81.868 | 33.498 | â | â | â | â |
| Zhang et al. | 2024 | 81.892 | 33.515 | â | â | â | â |
| Hunt & Reffert | 2024 | 81.892 | 33.515 | 0.455 | 0.34 | -2.779 | 54.256 |
| Cavallo et al. | 2024 | 81.91 | 33.536 | 0.455 | â | â | â |
| Hunt & Reffert | 2023 | 81.892 | 33.515 | 0.455 | 0.34 | -2.779 | 54.256 |
| Dias et al. | 2021 | 81.868 | 33.498 | 0.47 | 0.391 | -2.729 | â |
| Cantat-Gaudin et al. | 2020 | 81.874 | 33.526 | 0.47 | 0.393 | -2.762 | â |
| Cantat-Gaudin & Anders | 2020 | 81.874 | 33.526 | 0.47 | 0.393 | -2.762 | â |
| Monteiro & Dias | 2019 | 81.874 | 33.526 | â | â | â | 2.271 |
| Cantat-Gaudin et al. | 2019 | 81.874 | 33.526 | 0.47 | 0.39 | -2.73 | 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 | 1.995 | 1.105 | 1.0 | 144 | -0.095 | 228 | â | â |
| Li et al. | 2025 | 1.68 | 1.04 | â | 63 | -0.359 | â | â | â |
| Almeida et al. | 2025 | 1.92 | 1.17 | â | 144 | â | 189 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.095(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 268(1) | â | â |
| Cavallo et al. | 2024 | 1.99 | 0.89 | â | 479 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 2.01 | 0.81 | 1.00 | 214 | â | â | â | â |
| Dias et al. | 2021 | 1.92 | 1.17 | â | 144 | -0.133 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.00 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 2.17 | 1.23 | â | 67 | 0.014 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 2.00 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.