FSR 0591
(MWSC 196)
0.42
UTI
0.0
CN
0.06
Cdens
0.38
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
8.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.38 Low quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0591 is a sparse, very loose object of low 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, very young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 36.965 | 58.88 | 0.309 | -0.201 | -0.691 | â |
| Almeida et al. | 2025 | 36.932 | 58.763 | â | â | â | â |
| Hunt & Reffert | 2024 | 36.925 | 58.771 | 0.331 | -0.214 | -0.748 | -37.063 |
| Cavallo et al. | 2024 | 37.027 | 58.896 | 0.331 | â | â | â |
| He et al. | 2023 | 37.051 | 58.91 | 0.33 | -0.161 | -0.738 | -63.53 |
| Hunt & Reffert | 2023 | 36.925 | 58.771 | 0.331 | -0.214 | -0.748 | -37.063 |
| Almeida et al. | 2023 | 36.932 | 58.765 | â | â | â | â |
| Just et al. | 2023 | 36.904 | 58.755 | â | â | â | â |
| Dias et al. | 2021 | 36.932 | 58.763 | 0.293 | -0.232 | -0.562 | -72.562 |
| Bica et al. | 2019 | 36.929 | 58.759 | â | â | â | â |
| Kharchenko et al. | 2016 | 36.904 | 58.755 | â | â | â | â |
| Dias et al. | 2014 | 36.933 | 58.759 | â | 0.57 | 0.35 | â |
| Kharchenko et al. | 2013 | 36.915 | 58.758 | â | -0.98 | 1.52 | â |
| Kharchenko et al. | 2012 | 36.915 | 58.758 | â | -0.07 | 0.99 | â |
| Froebrich et al. | 2007 | 36.933 | 58.759 | â | â | â | â |
| Dias et al. | 2002 | 36.933 | 58.759 | â | 0.57 | 0.35 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.93 | 2.27 | â | 10 | â | 652 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1205* | â | â |
| Cavallo et al. | 2024 | 2.92 | 2.27 | â | 13 | 0.320 | â | â | â |
| He et al. | 2023 | 3.55 | 2.85 | â | 6 | â | â | â | â |
| Hunt & Reffert | 2023 | 2.72 | 2.47 | 2.39 | 17 | â | â | â | â |
| Almeida et al. | 2023 | 2.35 | 2.20 | â | 17 | -0.115 | 403* | 0.55 | â |
| Just et al. | 2023 | â | â | â | 7 | â | 115 | â | â |
| Dias et al. | 2021 | 2.93 | 2.27 | â | 10 | -0.187 | â | â | â |
| Kharchenko et al. | 2016 | 2.30 | 1.87 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.30 | 1.87 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.20 | 3.87 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 2.20 | 3.87 | â | 891 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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