FSR 0932
(SAI 57; MWSC 719)
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
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 91.092 | 14.575 | 0.448 | -0.442 | -0.833 | â |
| Almeida et al. | 2025 | 91.087 | 14.581 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.094 | 14.575 | 0.458 | -0.446 | -0.843 | â |
| Cavallo et al. | 2024 | 91.08 | 14.569 | 0.458 | â | â | â |
| Hunt & Reffert | 2023 | 91.094 | 14.575 | 0.458 | -0.446 | -0.843 | â |
| Just et al. | 2023 | 91.102 | 14.563 | â | â | â | â |
| Dias et al. | 2021 | 91.087 | 14.581 | 0.363 | -0.3 | -0.741 | â |
| Cantat-Gaudin et al. | 2020 | 91.087 | 14.573 | 0.402 | -0.36 | -0.789 | â |
| Zhong et al. | 2020 | 91.087 | 14.573 | â | -0.36 | -0.789 | 29.24 |
| Cantat-Gaudin & Anders | 2020 | 91.087 | 14.573 | 0.402 | -0.36 | -0.789 | â |
| Bica et al. | 2019 | 91.095 | 14.575 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 91.087 | 14.573 | 0.402 | -0.36 | -0.789 | â |
| Loktin & Popova | 2017 | 91.11 | 14.573 | â | -0.528 | -0.873 | â |
| Kharchenko et al. | 2016 | 91.102 | 14.563 | â | â | â | â |
| Dias et al. | 2014 | 91.092 | 14.573 | â | -3.72 | -3.01 | â |
| Kharchenko et al. | 2013 | 91.11 | 14.562 | â | -2.02 | -1.61 | â |
| Glushkova et al. | 2010 | 91.09 | 14.573 | â | â | â | â |
| Froebrich et al. | 2007 | 91.1 | 14.562 | â | â | â | â |
| Dias et al. | 2002 | 91.092 | 14.573 | â | -3.72 | -3.01 | 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 | 1.99 | 2.5 | 1.97 | 538 | 0.000 | 276 | â | â |
| Almeida et al. | 2025 | 2.00 | 3.02 | â | 68 | â | 276 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 496(1) | â | â |
| Cavallo et al. | 2024 | 1.82 | 3.11 | â | 69 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 1.99 | 3.26 | 1.97 | 71 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1259 | â | 20 | â | â |
| Dias et al. | 2021 | 2.00 | 3.02 | â | 68 | -0.142 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.34 | 2.82 | â | 117 | â | â | â | â |
| Zhong et al. | 2020 | 1.51 | 2.00 | â | 9100 | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.32 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.32 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.82 | 2.50 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.51 | 2.00 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.51 | 2.00 | â | 1259 | â | â | â | â |
| Glushkova et al. | 2010 | 1.09 | 1.21 | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 1.09 | 1.21 | â | 794 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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