FSR 1211
(MWSC 1312)
0.85
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
4.2 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1211 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, 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 absorption parameter (see Parameters). It is well-studied in the literature.
Distant
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 115.334 | -9.612 | 0.279 | -3.137 | 2.584 | 84.176 |
| Li et al. | 2025 | 115.336 | -9.607 | 0.288 | -3.137 | 2.564 | â |
| Hu & Soubiran | 2025 | 115.328 | -9.61 | â | â | â | â |
| Almeida et al. | 2025 | 115.338 | -9.604 | â | â | â | â |
| Hunt & Reffert | 2024 | 115.338 | -9.617 | 0.284 | -3.151 | 2.574 | 83.063 |
| Cavallo et al. | 2024 | 115.328 | -9.61 | 0.275 | â | â | â |
| Hunt & Reffert | 2023 | 115.338 | -9.617 | 0.284 | -3.151 | 2.574 | 83.063 |
| Almeida et al. | 2023 | 115.338 | -9.607 | â | â | â | â |
| Just et al. | 2023 | 115.374 | -9.608 | â | â | â | â |
| Dias et al. | 2021 | 115.338 | -9.604 | 0.291 | -3.122 | 2.556 | â |
| Cantat-Gaudin et al. | 2020 | 115.336 | -9.607 | 0.288 | -3.137 | 2.564 | â |
| Cantat-Gaudin & Anders | 2020 | 115.336 | -9.607 | 0.288 | -3.137 | 2.564 | â |
| Bossini et al. | 2019 | 115.336 | -9.607 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 115.336 | -9.607 | 0.288 | -3.137 | 2.564 | â |
| Kharchenko et al. | 2016 | 115.374 | -9.608 | â | â | â | â |
| Kharchenko et al. | 2013 | 115.38 | -9.61 | â | 2.24 | -1.23 | â |
| Froebrich et al. | 2007 | 115.362 | -9.615 | 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 | 3.28 | 0.53 | â | 1226 | -0.223 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270* | â | â | â |
| Almeida et al. | 2025 | 3.18 | 0.46 | â | 1334 | â | 259 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 574* | â | â |
| Cavallo et al. | 2024 | 2.63 | 0.26 | â | 1660 | -0.130 | â | â | â |
| Hunt & Reffert | 2023 | 3.06 | 0.14 | 0.58 | 1343 | â | â | â | â |
| Almeida et al. | 2023 | 3.07 | 0.03 | â | 1274 | 0.027 | 381* | 0.78 | â |
| Just et al. | 2023 | â | â | â | 1365 | â | 802 | â | â |
| Dias et al. | 2021 | 3.18 | 0.46 | â | 1334 | -0.185 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.31 | 0.19 | â | 1202 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.15 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 3.18 | 0.29 | â | 1067 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.15 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.33 | 0.16 | â | 1365 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.33 | 0.16 | â | 1365 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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