FSR 0932

(SAI 57; MWSC 719)

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0.82 UTI
0.38
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad) 40.0 [N/pc2]
  • CN 0.38 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.87 Well-studied
  • Cdup 1.0 Unique

Overview

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FSR 0932 is a poorly populated, very dense object of very 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, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.

Cavallo et al. (2024)
Gold sample.

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver 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– 91.092 14.575 0.448 -0.442 -0.833 –
Almeida et al. 2025 91.087 14.581 – – – –
Hunt & Reffert 2024 91.094 14.575 0.458 -0.446 -0.843 –
Cavallo et al. 2024 91.08 14.569 0.458 – – –
Hunt & Reffert 2023 91.094 14.575 0.458 -0.446 -0.843 –
Just et al. 2023 91.102 14.563 – – – –
Dias et al. 2021 91.087 14.581 0.363 -0.3 -0.741 –
Cantat-Gaudin et al. 2020 91.087 14.573 0.402 -0.36 -0.789 –
Zhong et al. 2020 91.087 14.573 – -0.36 -0.789 29.24
Cantat-Gaudin & Anders 2020 91.087 14.573 0.402 -0.36 -0.789 –
Bica et al. 2019 91.095 14.575 – – – –
Cantat-Gaudin et al. 2018 91.087 14.573 0.402 -0.36 -0.789 –
Loktin & Popova 2017 91.11 14.573 – -0.528 -0.873 –
Kharchenko et al. 2016 91.102 14.563 – – – –
Dias et al. 2014 91.092 14.573 – -3.72 -3.01 –
Kharchenko et al. 2013 91.11 14.562 – -2.02 -1.61 –
Glushkova et al. 2010 91.09 14.573 – – – –
Froebrich et al. 2007 91.1 14.562 – – – –
Dias et al. 2002 91.092 14.573 – -3.72 -3.01 –

💡 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– 1.99 2.5 1.97 538 0.000 276 – –
Almeida et al. 2025 2.00 3.02 – 68 – 276 – –
Hunt & Reffert 2024 – – – – – 496(1) – –
Cavallo et al. 2024 1.82 3.11 – 69 0.350 – – –
Hunt & Reffert 2023 1.99 3.26 1.97 71 – – – –
Just et al. 2023 – – – 1259 – 20 – –
Dias et al. 2021 2.00 3.02 – 68 -0.142 – – –
Cantat-Gaudin et al. 2020 2.34 2.82 – 117 – – – –
Zhong et al. 2020 1.51 2.00 – 9100 0.000 – – –
Cantat-Gaudin & Anders 2020 2.32 – – – – – – –
Cantat-Gaudin et al. 2018 2.32 – – – – – – –
Loktin & Popova 2017 2.82 2.50 – 282 – – – –
Kharchenko et al. 2016 1.51 2.00 – 1259 – – – –
Kharchenko et al. 2013 1.51 2.00 – 1259 – – – –
Glushkova et al. 2010 1.09 1.21 – 794 – – – –
Dias et al. 2002 1.09 1.21 – 794 – – – –

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

Visualization

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