FSR 0667

(Patchick 16; MWSC 341)

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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

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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.

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 –
Almeida et al. 2025 61.765 51.137 – – – –
Zhang et al. 2024 61.777 51.15 – – – –
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 – – –
Hunt & Reffert 2023 61.777 51.15 0.879 0.851 -3.757 -7.061
Almeida et al. 2023 61.769 51.142 – – – –
He et al. 2022 61.778 51.141 0.866 0.829 -3.731 –
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 –
Donor et al. 2020 61.807 51.167 – 0.64 -4.01 3.7
Cantat-Gaudin & Anders 2020 61.766 51.141 0.844 0.901 -3.87 –
Soubiran et al. 2018 61.766 51.141 – – – 2.5
Bica et al. 2019 61.788 51.175 – – – –
Cantat-Gaudin et al. 2018 61.766 51.141 0.844 0.901 -3.87 –
Dias et al. 2014 61.788 51.172 – 0.72 -1.86 –
Froebrich et al. 2007 61.788 51.172 – – – –
Dias et al. 2002 61.788 51.172 – -0.66 -1.05 –

💡 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 99999– 1.14 1.64 1.19 425 -0.013 119 0.57 –
Li et al. 2025 1.24 1.46 – 417 -0.006 – – –
Almeida et al. 2025 1.10 1.64 – 433 – 119 – –
Zhang et al. 2024 – – – – -0.244(1) – – –
Hunt & Reffert 2024 – – – – – 256(1) – –
Cavallo et al. 2024 1.17 1.37 – 479 0.230 – – –
Hunt & Reffert 2023 1.10 1.48 1.19 324 – – – –
Almeida et al. 2023 1.10 1.69 – 412 -0.111 115(1) 0.57 –
He et al. 2022 – 1.75 – 282 – – – –
Tarricq et al. 2022 1.14 – – 759 – – – –
Dias et al. 2021 1.10 1.64 – 433 0.047 – – –
Cantat-Gaudin et al. 2020 1.18 1.12 – 708 – – – –
Donor et al. 2020 – – – – -0.020 – – –
Cantat-Gaudin & Anders 2020 1.14 – – – – – – –
Soubiran et al. 2018 1.14 – – – – – – –
Cantat-Gaudin et al. 2018 1.14 – – – – – – –
Dias et al. 2002 1.82 2.90 – 120 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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