FSR 0558
(MWSC 157)
0.78
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
9.6 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0558 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (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 | 30.183 | 67.797 | 0.32 | -1.053 | 0.74 | -51.15 |
| Hunt & Reffert | 2024 | 30.147 | 67.792 | 0.338 | -1.058 | 0.718 | -26.688 |
| Cavallo et al. | 2024 | 30.185 | 67.793 | 0.336 | â | â | â |
| Hunt & Reffert | 2023 | 30.147 | 67.792 | 0.338 | -1.058 | 0.718 | -26.688 |
| Just et al. | 2023 | 30.117 | 67.801 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 30.191 | 67.799 | 0.314 | -1.024 | 0.794 | â |
| Cantat-Gaudin & Anders | 2020 | 30.191 | 67.799 | 0.314 | -1.024 | 0.794 | â |
| Soubiran et al. | 2018 | 30.191 | 67.799 | â | â | â | -48.85 |
| Bica et al. | 2019 | 30.198 | 67.803 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 30.191 | 67.799 | 0.314 | -1.024 | 0.794 | â |
| Kharchenko et al. | 2016 | 30.117 | 67.801 | â | â | â | â |
| Kharchenko et al. | 2013 | 30.13 | 67.803 | â | -2.89 | -1.47 | â |
| Kharchenko et al. | 2012 | 30.13 | 67.803 | â | -2.89 | -1.47 | â |
| Froebrich et al. | 2007 | 30.188 | 67.806 | 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 | 2.91 | 3.1 | 2.69 | 631 | 0.400 | 782 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1428(1) | â | â |
| Cavallo et al. | 2024 | 3.70 | 3.97 | â | 71 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 2.77 | 3.92 | 2.69 | 129 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 631 | â | 136 | â | â |
| Cantat-Gaudin et al. | 2020 | 2.91 | 2.52 | â | 537 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.92 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.92 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.92 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.50 | 3.10 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.50 | 3.10 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.50 | 3.10 | â | 631 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.