FSR 0942

(SAI 59; MWSC 729; FoF 681)

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0.91 UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 20.3 [N/pc2]
  • CN 0.8 Rich
  • 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 0942 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.

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– 91.496 13.667 0.307 -0.441 0.08 31.74
Hu & Soubiran 2025 91.482 13.661 – – – –
Zhang et al. 2024 91.506 13.67 – – – –
Hunt & Reffert 2024 91.506 13.67 0.311 -0.428 0.078 44.572
Cavallo et al. 2024 91.482 13.661 0.314 – – –
Hunt & Reffert 2023 91.506 13.67 0.311 -0.428 0.078 44.572
Just et al. 2023 91.487 13.661 – – – –
Cantat-Gaudin et al. 2020 91.487 13.667 0.277 -0.412 0.092 –
SΓ‘nchez et al. 2020 91.496 13.664 – -0.408 0.021 –
Donor et al. 2020 91.496 13.66 – -0.46 0.22 29.3
Cantat-Gaudin & Anders 2020 91.487 13.667 0.277 -0.412 0.092 –
Liu & Pang 2019 91.493 13.675 0.3 -0.346 0.084 –
Soubiran et al. 2018 91.487 13.667 – – – 31.88
Bica et al. 2019 91.51 13.668 – – – –
Cantat-Gaudin et al. 2018 91.487 13.667 0.277 -0.412 0.092 –
Loktin & Popova 2017 91.5 13.659 – -0.434 -0.506 –
Kharchenko et al. 2016 91.487 13.661 – – – –
Dias et al. 2014 91.496 13.664 – -3.92 -2.28 –
Kharchenko et al. 2013 91.495 13.66 – -0.98 -1.77 –
Glushkova et al. 2010 91.497 13.664 – – – –
Froebrich et al. 2007 91.492 13.668 – – – –
Dias et al. 2002 91.496 13.664 – -3.92 -2.28 –

πŸ’‘ 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– 3.16 1.935 2.22 1000 -0.255 844 – –
Hu & Soubiran 2025 – – – – -0.230(5) – – –
Zhang et al. 2024 – – – – -0.379(1) – – –
Hunt & Reffert 2024 – – – – – 1352(1) – –
Cavallo et al. 2024 3.16 2.51 – 501 0.310 – – –
Hunt & Reffert 2023 2.90 2.06 2.22 574 – – – –
Just et al. 2023 – – – 1000 – 337 – –
Cantat-Gaudin et al. 2020 3.40 1.73 – 724 – – – –
Donor et al. 2020 – – – – -0.280 – – –
Cantat-Gaudin & Anders 2020 3.27 – – – – – – –
Liu & Pang 2019 – – – 1100 0.500 – – –
Soubiran et al. 2018 3.27 – – – – – – –
Cantat-Gaudin et al. 2018 3.27 – – – – – – –
Loktin & Popova 2017 3.61 1.87 – 316 – – – –
Kharchenko et al. 2016 2.08 2.00 – 1000 – – – –
Kharchenko et al. 2013 2.08 2.00 – 1000 – – – –
Glushkova et al. 2010 2.00 1.83 – 1000 – – – –
Dias et al. 2002 2.00 1.83 – 1000 -0.290 – – –

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

Visualization

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