COIN-Gaia 6
(COIN 6; FoF 74)
0.78
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
13.8 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 6 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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 | 28.101 | 58.641 | 0.295 | -2.355 | -0.473 | -42.314 |
| Li et al. | 2025 | 28.101 | 58.636 | 0.277 | -2.355 | -0.49 | â |
| Hu & Soubiran | 2025 | 28.097 | 58.641 | â | â | â | â |
| Almeida et al. | 2025 | 28.082 | 58.625 | â | â | â | â |
| Hunt & Reffert | 2024 | 28.138 | 58.635 | 0.299 | -2.346 | -0.483 | -42.596 |
| Cavallo et al. | 2024 | 28.097 | 58.641 | 0.296 | â | â | â |
| Hunt & Reffert | 2023 | 28.138 | 58.635 | 0.299 | -2.346 | -0.483 | -42.596 |
| Dias et al. | 2021 | 28.082 | 58.625 | 0.272 | -2.382 | -0.484 | -42.341 |
| Cantat-Gaudin et al. | 2020 | 28.101 | 58.636 | 0.277 | -2.355 | -0.49 | â |
| Cantat-Gaudin & Anders | 2020 | 28.101 | 58.636 | 0.277 | -2.355 | -0.49 | â |
| Liu & Pang | 2019 | 28.234 | 58.626 | 0.271 | -2.037 | -0.389 | â |
| Monteiro & Dias | 2019 | 28.101 | 58.636 | â | â | â | 2.138 |
| Cantat-Gaudin et al. | 2019 | 28.101 | 58.636 | 0.28 | -2.35 | -0.44 | 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 | 3.06 | 1.53 | 0.75 | 585 | -0.154 | 726 | â | â |
| Li et al. | 2025 | 3.15 | 1.32 | â | 679 | -0.039 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.180(5) | â | â | â |
| Almeida et al. | 2025 | 2.90 | 1.56 | â | 585 | â | 601 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 852(1) | â | â |
| Cavallo et al. | 2024 | 2.59 | 1.53 | â | 661 | -0.300 | â | â | â |
| Hunt & Reffert | 2023 | 3.05 | 1.15 | 0.75 | 537 | â | â | â | â |
| Dias et al. | 2021 | 2.90 | 1.56 | â | 585 | -0.129 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.27 | 1.18 | â | 479 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.27 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1100 | -0.250 | â | â | â |
| Monteiro & Dias | 2019 | 3.06 | 2.18 | â | 50 | 0.003 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 3.27 | 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: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.