FSR 0166
(MWSC 3286; FoF 47)
0.93
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
5.4 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0166 is a very rich, 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 massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 303.381 | 25.427 | 0.324 | -4.172 | -6.67 | -10.791 |
| Li et al. | 2025 | 303.385 | 25.43 | 0.331 | -4.191 | -6.659 | â |
| Hu & Soubiran | 2025 | 303.379 | 25.42 | â | â | â | â |
| Hunt & Reffert | 2024 | 303.406 | 25.43 | 0.329 | -4.168 | -6.668 | -11.412 |
| Cavallo et al. | 2024 | 303.379 | 25.42 | 0.325 | â | â | â |
| Hunt & Reffert | 2023 | 303.406 | 25.43 | 0.329 | -4.168 | -6.668 | -11.412 |
| Just et al. | 2023 | 303.394 | 25.453 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 303.385 | 25.43 | 0.331 | -4.191 | -6.659 | â |
| Cantat-Gaudin & Anders | 2020 | 303.385 | 25.43 | 0.331 | -4.191 | -6.659 | â |
| Liu & Pang | 2019 | 303.39 | 25.425 | 0.329 | -4.14 | -6.649 | â |
| Soubiran et al. | 2018 | 303.385 | 25.43 | â | â | â | -12.36 |
| Bica et al. | 2019 | 303.41 | 25.454 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 303.385 | 25.43 | 0.331 | -4.191 | -6.659 | â |
| Kharchenko et al. | 2016 | 303.394 | 25.453 | â | â | â | â |
| Kharchenko et al. | 2013 | 303.4 | 25.455 | â | -3.37 | -3.34 | â |
| Froebrich et al. | 2007 | 303.408 | 25.455 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.15 | 2.48 | â | 5912 | -0.041 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | 0.030* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3708* | â | â |
| Cavallo et al. | 2024 | 2.54 | 2.73 | â | 2692 | -0.300 | â | â | â |
| Hunt & Reffert | 2023 | 2.80 | 2.75 | 1.81 | 1102 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1109 | â | 247 | â | â |
| Cantat-Gaudin et al. | 2020 | 2.81 | 2.24 | â | 2818 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.77 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 2950 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 2.77 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.77 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.90 | 2.90 | â | 1109 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.90 | 2.90 | â | 1109 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.