COIN-Gaia 3
(COIN 3)
0.76
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
6.5 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 3 is a rich, very dense object of high 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 metallicity parameter (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.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 18.734 | 60.504 | 0.797 | -2.461 | -1.885 | -34.42 |
| Almeida et al. | 2025 | 18.745 | 60.501 | â | â | â | â |
| Hunt & Reffert | 2024 | 18.727 | 60.507 | 0.794 | -2.458 | -1.887 | -29.907 |
| Cavallo et al. | 2024 | 18.765 | 60.491 | 0.796 | â | â | â |
| Hunt & Reffert | 2023 | 18.727 | 60.507 | 0.794 | -2.458 | -1.887 | -29.907 |
| Almeida et al. | 2023 | 18.722 | 60.48 | â | â | â | â |
| Tarricq et al. | 2022 | 18.773 | 60.493 | 0.794 | -2.463 | -1.866 | â |
| Dias et al. | 2021 | 18.745 | 60.501 | 0.789 | -2.44 | -1.793 | -40.543 |
| Cantat-Gaudin et al. | 2020 | 18.739 | 60.505 | 0.775 | -2.431 | -1.791 | â |
| Cantat-Gaudin & Anders | 2020 | 18.739 | 60.505 | 0.775 | -2.431 | -1.791 | â |
| Monteiro & Dias | 2019 | 18.739 | 60.505 | â | â | â | 2.938 |
| Cantat-Gaudin et al. | 2019 | 18.739 | 60.505 | 0.78 | -2.43 | -1.81 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.10 | 1.92 | â | 99 | â | 365 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 510* | â | â |
| Cavallo et al. | 2024 | 1.50 | 1.98 | â | 141 | 0.780 | â | â | â |
| Hunt & Reffert | 2023 | 1.21 | 2.19 | 2.58 | 91 | â | â | â | â |
| Almeida et al. | 2023 | 1.15 | 1.97 | â | 105 | 0.251 | 350* | 0.63 | â |
| Tarricq et al. | 2022 | 1.18 | â | â | 59 | â | â | â | â |
| Dias et al. | 2021 | 1.10 | 1.92 | â | 99 | 0.082 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.21 | 1.69 | â | 49 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.24 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.11 | 1.51 | â | 38 | 0.033 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 1.24 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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