COIN-Gaia 28
(COIN 28)
0.76
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
5.5 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 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.
Relatively close
Low 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 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.53 | 1.13 | â | 53 | â | 324 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.009* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 321* | 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* | 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 |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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