FSR 1083
(MWSC 1192; Kronberger 97)
0.85
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
9.8 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1083 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old 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 | 110.503 | 3.557 | 0.189 | -0.354 | 0.244 | 101.715 |
| Li et al. | 2025 | 110.503 | 3.557 | 0.191 | -0.331 | 0.245 | â |
| Hu & Soubiran | 2025 | 110.507 | 3.555 | â | â | â | â |
| Almeida et al. | 2025 | 110.507 | 3.553 | â | â | â | â |
| Zhang et al. | 2024 | 110.516 | 3.556 | â | â | â | â |
| Hunt & Reffert | 2024 | 110.516 | 3.556 | 0.193 | -0.359 | 0.233 | 98.044 |
| Cavallo et al. | 2024 | 110.506 | 3.555 | 0.191 | â | â | â |
| Hunt & Reffert | 2023 | 110.516 | 3.556 | 0.193 | -0.359 | 0.233 | 98.044 |
| Just et al. | 2023 | 110.505 | 3.582 | â | â | â | â |
| Dias et al. | 2021 | 110.507 | 3.553 | 0.189 | -0.352 | 0.292 | 98.162 |
| Cantat-Gaudin et al. | 2020 | 110.503 | 3.557 | 0.191 | -0.331 | 0.245 | â |
| Cantat-Gaudin & Anders | 2020 | 110.503 | 3.557 | 0.191 | -0.331 | 0.245 | â |
| Soubiran et al. | 2018 | 110.503 | 3.557 | â | â | â | 98.56 |
| Bica et al. | 2019 | 110.511 | 3.583 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 110.503 | 3.557 | 0.191 | -0.331 | 0.245 | â |
| Kharchenko et al. | 2016 | 110.505 | 3.582 | â | â | â | â |
| Kharchenko et al. | 2013 | 110.512 | 3.58 | â | -1.74 | 1.83 | â |
| Froebrich et al. | 2007 | 110.504 | 3.58 | â | â | â | 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 | 4.54 | 0.455 | 1.65 | 1995 | -0.258 | 761 | â | â |
| Li et al. | 2025 | 4.80 | 0.51 | â | 2664 | -0.258 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.200(5) | â | â | â |
| Almeida et al. | 2025 | 4.29 | 0.37 | â | 3483 | â | 761 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.462(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 774(1) | â | â |
| Cavallo et al. | 2024 | 3.42 | 0.48 | â | 3162 | -0.400 | â | â | â |
| Hunt & Reffert | 2023 | 4.55 | 0.29 | 1.65 | 1227 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 646 | â | 58 | â | â |
| Dias et al. | 2021 | 4.29 | 0.37 | â | 3483 | -0.103 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.88 | 0.43 | â | 1995 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.54 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.54 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.54 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.77 | 2.45 | â | 646 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.77 | 2.45 | â | 646 | 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: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.