COIN-Gaia 28
(COIN 28)
0.74
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
21.2 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 28 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 low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a large 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 | 96.329 | 11.158 | 0.592 | -1.125 | -0.962 | 29.717 |
| Almeida et al. | 2025 | 96.353 | 11.15 | â | â | â | â |
| Zhang et al. | 2024 | 96.331 | 11.163 | â | â | â | â |
| Hunt & Reffert | 2024 | 96.331 | 11.163 | 0.596 | -1.151 | -0.977 | 9.903 |
| Cavallo et al. | 2024 | 96.323 | 11.164 | 0.595 | â | â | â |
| Hunt & Reffert | 2023 | 96.331 | 11.163 | 0.596 | -1.151 | -0.977 | 9.903 |
| Almeida et al. | 2023 | 96.339 | 11.145 | â | â | â | â |
| Dias et al. | 2021 | 96.353 | 11.15 | 0.61 | -1.134 | -0.943 | â |
| Cantat-Gaudin et al. | 2020 | 96.333 | 11.159 | 0.59 | -1.12 | -0.942 | â |
| Cantat-Gaudin & Anders | 2020 | 96.333 | 11.159 | 0.59 | -1.12 | -0.942 | â |
| Monteiro & Dias | 2019 | 96.333 | 11.159 | â | â | â | 3.082 |
| Cantat-Gaudin et al. | 2019 | 96.333 | 11.159 | 0.59 | -1.12 | -0.94 | 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 | 1.54 | 0.96 | 0.83 | 60 | -0.047 | 324 | 0.39 | â |
| Almeida et al. | 2025 | 1.53 | 1.13 | â | 53 | â | 324 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.009(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 321(1) | â | â |
| Cavallo et al. | 2024 | 1.55 | 0.96 | â | 132 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 1.54 | 0.80 | 0.83 | 121 | â | â | â | â |
| Almeida et al. | 2023 | 1.49 | 1.07 | â | 90 | -0.105 | 388(1) | 0.39 | â |
| Dias et al. | 2021 | 1.53 | 1.13 | â | 53 | -0.047 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.60 | 0.75 | â | 55 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.62 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.52 | 0.85 | â | 60 | 0.007 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 1.62 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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