COIN-Gaia 1
(COIN 1)
0.75
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
18.3 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 1 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age 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 | – | 11.82 | 66.747 | 1.552 | -5.04 | -3.146 | -14.34 |
| Almeida et al. | 2025 | 11.999 | 66.782 | – | – | – | – |
| Alfonso et al. | 2024 | 11.803 | 66.687 | 1.51 | -5.006 | -3.114 | – |
| He et al. | 2022 | 11.986 | 66.757 | 1.552 | -5.023 | -3.137 | – |
| Dias et al. | 2021 | 11.999 | 66.782 | 1.547 | -5.021 | -3.047 | – |
| Cantat-Gaudin et al. | 2020 | 11.933 | 66.769 | 1.546 | -5.034 | -3.048 | – |
| Monteiro & Dias | 2019 | 11.933 | 66.769 | – | – | – | 2.687 |
| Cantat-Gaudin et al. | 2019 | 11.933 | 66.769 | 1.55 | -5.03 | -3.04 | – |
💡 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 | 0.64 | 1.62 | – | 239 | – | 201 | – | – |
| Alfonso et al. | 2024 | 0.66 | 1.13 | – | 224 | 0.035 | – | – | – |
| He et al. | 2022 | – | 1.80 | – | 112 | – | – | – | – |
| Tarricq et al. | 2022 | 0.65 | – | – | 200 | – | – | – | – |
| Dias et al. | 2021 | 0.64 | 1.62 | – | 239 | 0.035 | – | – | – |
| Cantat-Gaudin et al. | 2020 | 0.66 | 1.13 | – | 182 | – | – | – | – |
| Monteiro & Dias | 2019 | 0.67 | 1.29 | – | 543 | 0.036 | – | – | – |
| Cantat-Gaudin et al. | 2019 | 0.64 | – | – | – | – | – | – | – |
💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
