FSR 0811
(MWSC 826)
0.58
UTI
0.3
CN
0.43
Cdens
1.0
CC3
0.58
Clit
1.0
Cdup
Nm (P>50%)
30
Core radius and density
1.1 [pc], 2.1 [pc-2]
- CN 0.3 Poorly populated
- Cdens 0.43 Loose
- CC3 1.0 Very high quality
- Clit 0.58 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0811 is a poorly populated, loose object of very 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, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 94.122 | 36.379 | 0.343 | 0.903 | -2.049 | 29.879 |
| Hu & Soubiran | 2025 | 94.116 | 36.386 | â | â | â | â |
| Almeida et al. | 2025 | 94.095 | 36.38 | â | â | â | â |
| Zhang et al. | 2024 | 94.113 | 36.364 | â | â | â | â |
| Hunt & Reffert | 2024 | 94.113 | 36.364 | 0.34 | 0.906 | -2.033 | 29.871 |
| Cavallo et al. | 2024 | 94.116 | 36.386 | 0.341 | â | â | â |
| Hunt & Reffert | 2023 | 94.113 | 36.364 | 0.34 | 0.906 | -2.033 | 29.871 |
| Almeida et al. | 2023 | 94.097 | 36.378 | â | â | â | â |
| Just et al. | 2023 | 94.093 | 36.367 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 94.105 | 36.377 | â | â | â | â |
| Dias et al. | 2021 | 94.095 | 36.38 | 0.339 | 0.958 | -2.096 | â |
| Cantat-Gaudin et al. | 2020 | 94.105 | 36.377 | 0.325 | 0.948 | -2.064 | â |
| Zhong et al. | 2020 | 94.105 | 36.377 | â | 0.948 | -2.064 | -6.142 |
| Cantat-Gaudin & Anders | 2020 | 94.105 | 36.377 | 0.325 | 0.948 | -2.064 | â |
| Bica et al. | 2019 | 94.081 | 36.356 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 94.105 | 36.377 | 0.325 | 0.948 | -2.064 | â |
| Kharchenko et al. | 2016 | 94.093 | 36.367 | â | â | â | â |
| Kharchenko et al. | 2013 | 94.102 | 36.365 | â | -3.02 | 1.6 | â |
| Kharchenko et al. | 2012 | 94.102 | 36.365 | â | -3.02 | 1.6 | â |
| Froebrich et al. | 2007 | 94.083 | 36.355 | 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 | 2.82 | 0.915 | 0.665 | 631 | -0.164 | 266 | 0.57 | 0 |
| Hu & Soubiran | 2025 | â | â | â | â | -0.220(5) | â | â | â |
| Almeida et al. | 2025 | 2.35 | 1.00 | â | 590 | â | 262 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.232(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.56 | 0.57 | 0.66 | 462 | â | 266(1) | â | â |
| Cavallo et al. | 2024 | 2.49 | 0.93 | â | 871 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 2.56 | 0.57 | 0.67 | 462 | â | â | â | â |
| Almeida et al. | 2023 | 2.47 | 0.90 | â | 776 | -0.131 | 239(1) | 0.57 | â |
| Just et al. | 2023 | â | â | â | 631 | â | 968 | â | â |
| Jadhav & Subramaniam | 2021 | 3.09 | 0.88 | â | 407 | â | 357 | â | 0(1) |
| Dias et al. | 2021 | 2.35 | 1.00 | â | 590 | -0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.09 | 0.88 | â | 407 | â | â | â | â |
| Kounkel et al. | 2020 | 2.83 | 0.84 | â | 891 | â | â | â | â |
| Zhong et al. | 2020 | 2.82(1) | â | â | â | -0.187 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.82 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.82 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 5.44 | 1.18 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.44 | 1.18 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2012 | 5.44 | 1.18 | â | 631 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.3249, e_all=0.0698.