COIN-Gaia 11
(COIN 11; UBC 60)
0.81
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.64
Clit
1.0
Cdup
Stellar density (N50/rad)
11.4 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.64 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 11 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close 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 metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 68.101 | 39.493 | 1.518 | 3.492 | -5.72 | -6.237 |
| Bijavara Seshashayana et al. | 2025 | 68.068 | 39.515 | â | â | â | â |
| Li et al. | 2025 | 68.11 | 39.479 | 1.485 | 3.574 | -5.62 | â |
| Almeida et al. | 2025 | 68.08 | 39.484 | â | â | â | â |
| Alfonso et al. | 2024 | 68.113 | 39.515 | 1.468 | 3.45 | -5.722 | â |
| Zhang et al. | 2024 | 68.15 | 39.533 | â | â | â | â |
| Hunt & Reffert | 2024 | 68.15 | 39.533 | 1.517 | 3.437 | -5.748 | -4.943 |
| Cavallo et al. | 2024 | 68.111 | 39.569 | 1.517 | â | â | â |
| Hunt & Reffert | 2023 | 68.15 | 39.533 | 1.517 | 3.437 | -5.748 | -4.943 |
| Almeida et al. | 2023 | 68.058 | 39.516 | â | â | â | â |
| He et al. | 2022 | 68.124 | 39.52 | 1.516 | 3.458 | -5.734 | â |
| Tarricq et al. | 2022 | 68.11 | 39.503 | 1.492 | 3.459 | -5.748 | â |
| Jadhav & Subramaniam | 2021 | 68.11 | 39.479 | â | â | â | â |
| Dias et al. | 2021 | 68.08 | 39.484 | 1.489 | 3.58 | -5.628 | 0.162 |
| Cantat-Gaudin et al. | 2020 | 68.11 | 39.479 | 1.485 | 3.574 | -5.62 | â |
| Cantat-Gaudin & Anders | 2020 | 68.11 | 39.479 | 1.485 | 3.574 | -5.62 | â |
| Castro-Ginard et al. | 2019 | 68.134 | 39.497 | 1.469 | 3.619 | -5.734 | â |
| Monteiro & Dias | 2019 | 68.11 | 39.479 | â | â | â | 2.729 |
| Cantat-Gaudin et al. | 2019 | 68.11 | 39.479 | 1.49 | 3.57 | -5.63 | 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 | 0.66 | 1.57 | 2.08 | 661 | 0.053 | 296 | 0.69 | 1 |
| Bijavara Seshashayana et al. | 2025 | â | 1.25 | â | 790 | 0.130(14) | â | â | â |
| Li et al. | 2025 | 0.65 | 1.52 | â | 752 | 0.150 | â | â | â |
| Almeida et al. | 2025 | 0.64 | 1.77 | â | 627 | â | 234 | â | â |
| Alfonso et al. | 2024 | 0.67 | 1.25 | â | 795 | 0.047 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.059(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 287(1) | â | â |
| Cavallo et al. | 2024 | 0.66 | 1.89 | â | 490 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.62 | 1.77 | 2.08 | 339 | â | â | â | â |
| Almeida et al. | 2023 | 0.64 | 1.88 | â | 566 | -0.001 | 332(1) | 0.69 | â |
| He et al. | 2022 | â | 2.15 | â | 355 | â | â | â | â |
| Tarricq et al. | 2022 | 0.67 | â | â | 794 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 0.67 | 1.25 | â | 794 | â | 304 | â | 1(1) |
| Dias et al. | 2021 | 0.64 | 1.77 | â | 627 | 0.047 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.67 | 1.25 | â | 794 | â | â | â | â |
| Kounkel et al. | 2020 | 0.69 | 1.57 | â | 603 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.66 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.64 | 1.31 | â | 695 | 0.023 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.66 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G18, along with HSC_1268 and HSC_1291.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).