FSR 0667
(Patchick 16; MWSC 341)
0.88
UTI
0.66
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
10.7 [N/pc2]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0667 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively 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 very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 61.768 | 51.146 | 0.863 | 0.853 | -3.748 | -0.512 |
| Li et al. | 2025 | 61.766 | 51.141 | 0.844 | 0.901 | -3.87 | â |
| Almeida et al. | 2025 | 61.765 | 51.137 | â | â | â | â |
| Zhang et al. | 2024 | 61.777 | 51.15 | â | â | â | â |
| Hunt & Reffert | 2024 | 61.777 | 51.15 | 0.879 | 0.851 | -3.757 | -7.061 |
| Cavallo et al. | 2024 | 61.752 | 51.13 | 0.874 | â | â | â |
| Hunt & Reffert | 2023 | 61.777 | 51.15 | 0.879 | 0.851 | -3.757 | -7.061 |
| Almeida et al. | 2023 | 61.769 | 51.142 | â | â | â | â |
| He et al. | 2022 | 61.778 | 51.141 | 0.866 | 0.829 | -3.731 | â |
| Dias et al. | 2021 | 61.765 | 51.137 | 0.843 | 0.922 | -3.877 | 1.838 |
| Cantat-Gaudin et al. | 2020 | 61.766 | 51.141 | 0.844 | 0.901 | -3.87 | â |
| Donor et al. | 2020 | 61.807 | 51.167 | â | 0.64 | -4.01 | 3.7 |
| Cantat-Gaudin & Anders | 2020 | 61.766 | 51.141 | 0.844 | 0.901 | -3.87 | â |
| Soubiran et al. | 2018 | 61.766 | 51.141 | â | â | â | 2.5 |
| Bica et al. | 2019 | 61.788 | 51.175 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 61.766 | 51.141 | 0.844 | 0.901 | -3.87 | â |
| Dias et al. | 2014 | 61.788 | 51.172 | â | 0.72 | -1.86 | â |
| Froebrich et al. | 2007 | 61.788 | 51.172 | â | â | â | â |
| Dias et al. | 2002 | 61.788 | 51.172 | â | -0.66 | -1.05 | 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 | 1.14 | 1.64 | 1.19 | 425 | -0.013 | 119 | 0.57 | â |
| Li et al. | 2025 | 1.24 | 1.46 | â | 417 | -0.006 | â | â | â |
| Almeida et al. | 2025 | 1.10 | 1.64 | â | 433 | â | 119 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.244(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 256(1) | â | â |
| Cavallo et al. | 2024 | 1.17 | 1.37 | â | 479 | 0.230 | â | â | â |
| Hunt & Reffert | 2023 | 1.10 | 1.48 | 1.19 | 324 | â | â | â | â |
| Almeida et al. | 2023 | 1.10 | 1.69 | â | 412 | -0.111 | 115(1) | 0.57 | â |
| He et al. | 2022 | â | 1.75 | â | 282 | â | â | â | â |
| Tarricq et al. | 2022 | 1.14 | â | â | 759 | â | â | â | â |
| Dias et al. | 2021 | 1.10 | 1.64 | â | 433 | 0.047 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.18 | 1.12 | â | 708 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.020 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.14 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.14 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.14 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.82 | 2.90 | â | 120 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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