COIN-Gaia 37
(COIN 37)
0.38
UTI
0.0
CN
0.17
Cdens
0.38
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
0.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.17 Very loose
- CC3 0.38 Low quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 37 is a sparse, very loose 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, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 45.439 | 58.27 | 0.978 | 0.849 | -2.094 | -51.137 |
| Li et al. | 2025 | 45.377 | 58.329 | 0.976 | 0.849 | -2.042 | â |
| Almeida et al. | 2025 | 44.996 | 58.443 | â | â | â | â |
| Hunt & Reffert | 2024 | 45.232 | 58.862 | 0.977 | 0.833 | -2.186 | -45.667 |
| Cavallo et al. | 2024 | 45.341 | 58.512 | 0.977 | â | â | â |
| Hunt & Reffert | 2023 | 45.232 | 58.862 | 0.977 | 0.833 | -2.186 | -45.667 |
| Almeida et al. | 2023 | 44.954 | 58.432 | â | â | â | â |
| He et al. | 2022 | 45.213 | 58.862 | 0.967 | 0.866 | -2.54 | â |
| Dias et al. | 2021 | 44.996 | 58.443 | 0.973 | 0.859 | -2.039 | â |
| Cantat-Gaudin et al. | 2020 | 45.377 | 58.329 | 0.976 | 0.849 | -2.042 | â |
| Cantat-Gaudin & Anders | 2020 | 45.377 | 58.329 | 0.976 | 0.849 | -2.042 | â |
| Monteiro & Dias | 2019 | 45.377 | 58.329 | â | â | â | 2.144 |
| Cantat-Gaudin et al. | 2019 | 45.377 | 58.329 | 0.98 | 0.85 | -2.04 | 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 | 2.01 | 0.83 | 26 | 0.063 | 150 | 0.7 | â |
| Li et al. | 2025 | 1.17 | 2.08 | â | 26 | 0.136 | â | â | â |
| Almeida et al. | 2025 | 0.96 | 1.94 | â | 26 | â | 155 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 74(1) | â | â |
| Cavallo et al. | 2024 | 1.10 | 2.07 | â | 18 | 0.430 | â | â | â |
| Hunt & Reffert | 2023 | 0.98 | 1.92 | 0.83 | 27 | â | â | â | â |
| Almeida et al. | 2023 | 0.97 | 1.96 | â | 109 | 0.046 | 150(1) | 0.70 | â |
| He et al. | 2022 | â | 2.50 | â | 50 | â | â | â | â |
| Dias et al. | 2021 | 0.96 | 1.94 | â | 26 | 0.063 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.99 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.05 | 2.06 | â | 85 | 0.020 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.99 | 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.