COIN-Gaia 34
(COIN 34)
0.78
UTI
0.59
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
10.8 [arcmin]
- CN 0.59 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 34 is a moderately populated, very dense object of 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 age parameter (see Parameters). It is well-studied in the literature.
Close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 31.216 | 61.777 | 1.038 | -2.28 | 0.802 | -25.114 |
| Li et al. | 2025 | 31.231 | 61.776 | 1.006 | -2.231 | 0.866 | â |
| Almeida et al. | 2025 | 31.235 | 61.784 | â | â | â | â |
| Alfonso et al. | 2024 | 31.038 | 61.845 | 1.025 | -2.225 | 0.716 | â |
| Hunt & Reffert | 2024 | 31.234 | 61.781 | 1.041 | -2.275 | 0.796 | -23.565 |
| Cavallo et al. | 2024 | 31.13 | 61.807 | 1.044 | â | â | â |
| Hunt & Reffert | 2023 | 31.234 | 61.781 | 1.041 | -2.275 | 0.796 | -23.565 |
| Almeida et al. | 2023 | 31.262 | 61.774 | â | â | â | â |
| He et al. | 2022 | 31.254 | 61.794 | 1.049 | -2.306 | 0.804 | â |
| Tarricq et al. | 2022 | 31.29 | 61.815 | 1.051 | -2.256 | 0.784 | â |
| Dias et al. | 2021 | 31.235 | 61.784 | 1.008 | -2.254 | 0.863 | â |
| Cantat-Gaudin et al. | 2020 | 31.231 | 61.776 | 1.006 | -2.231 | 0.866 | â |
| Cantat-Gaudin & Anders | 2020 | 31.231 | 61.776 | 1.006 | -2.231 | 0.866 | â |
| Monteiro & Dias | 2019 | 31.231 | 61.776 | â | â | â | 2.526 |
| Cantat-Gaudin et al. | 2019 | 31.231 | 61.776 | 1.01 | -2.23 | 0.88 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.85 | 1.95 | â | 42 | -0.130 | â | â | â |
| Almeida et al. | 2025 | 0.95 | 1.93 | â | 158 | â | 164 | â | â |
| Alfonso et al. | 2024 | 1.00 | 1.19 | â | 222 | -0.082 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 212* | â | â |
| Cavallo et al. | 2024 | 1.00 | 1.95 | â | 87 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 0.91 | 1.72 | 2.19 | 105 | â | â | â | â |
| Almeida et al. | 2023 | 0.97 | 1.94 | â | 75 | 0.029 | 79* | 0.68 | â |
| He et al. | 2022 | â | 2.25 | â | 50 | â | â | â | â |
| Tarricq et al. | 2022 | 1.00 | â | â | 245 | â | â | â | â |
| Dias et al. | 2021 | 0.95 | 1.93 | â | 158 | -0.084 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.02 | 1.19 | â | 219 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.97 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.05 | 1.67 | â | 96 | 0.022 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.97 | 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.