COIN-Gaia 7
(COIN 7)
0.75
UTI
0.72
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
9.9 [N/pc2]
- CN 0.72 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 7 is a moderately populated, 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 significant percentage of members with 2 later reported entries. 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 | 33.769 | 58.463 | 0.666 | -1.045 | -1.662 | â |
| Almeida et al. | 2025 | 33.712 | 58.443 | â | â | â | â |
| Hunt & Reffert | 2024 | 33.753 | 58.459 | 0.662 | -1.057 | -1.65 | â |
| Cavallo et al. | 2024 | 33.797 | 58.454 | 0.665 | â | â | â |
| Hunt & Reffert | 2023 | 33.753 | 58.459 | 0.662 | -1.057 | -1.65 | â |
| Almeida et al. | 2023 | 33.71 | 58.448 | â | â | â | â |
| Tarricq et al. | 2022 | 33.762 | 58.395 | 0.689 | -1.029 | -1.654 | â |
| Dias et al. | 2021 | 33.712 | 58.443 | 0.646 | -1.047 | -1.546 | â |
| Cantat-Gaudin et al. | 2020 | 33.738 | 58.466 | 0.648 | -1.043 | -1.548 | â |
| Cantat-Gaudin & Anders | 2020 | 33.738 | 58.466 | 0.648 | -1.043 | -1.548 | â |
| Monteiro & Dias | 2019 | 33.738 | 58.466 | â | â | â | 2.478 |
| Cantat-Gaudin et al. | 2019 | 33.738 | 58.466 | 0.65 | -1.04 | -1.56 | 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 | 1.455 | 1.68 | 1.36 | 87 | 0.057 | 254 | 0.48 | â |
| Almeida et al. | 2025 | 1.33 | 1.68 | â | 87 | â | 195 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 386(1) | â | â |
| Cavallo et al. | 2024 | 1.61 | 1.73 | â | 72 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 1.40 | 1.57 | 1.36 | 151 | â | â | â | â |
| Almeida et al. | 2023 | 1.35 | 1.72 | â | 107 | 0.002 | 254(1) | 0.48 | â |
| Tarricq et al. | 2022 | 1.43 | â | â | 62 | â | â | â | â |
| Dias et al. | 2021 | 1.33 | 1.68 | â | 87 | 0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.49 | 1.36 | â | 58 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.48 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.48 | 1.59 | â | 103 | 0.014 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 1.48 | 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.