FSR 0524
(SAI 11; MWSC 92)
0.84
UTI
0.73
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.73 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0524 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Distant
Moderate 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 | 14.335 | 62.118 | 0.247 | -1.601 | -0.286 | -81.33 |
| Almeida et al. | 2025 | 14.339 | 62.118 | â | â | â | â |
| Hunt & Reffert | 2024 | 14.318 | 62.121 | 0.25 | -1.608 | -0.284 | -75.803 |
| Cavallo et al. | 2024 | 14.338 | 62.111 | 0.242 | â | â | â |
| Hunt & Reffert | 2023 | 14.318 | 62.121 | 0.25 | -1.608 | -0.284 | -75.803 |
| Just et al. | 2023 | 14.31 | 62.122 | â | â | â | â |
| Dias et al. | 2021 | 14.339 | 62.118 | 0.216 | -1.584 | -0.212 | -79.419 |
| Cantat-Gaudin et al. | 2020 | 14.34 | 62.125 | 0.226 | -1.547 | -0.246 | â |
| Cantat-Gaudin & Anders | 2020 | 14.34 | 62.125 | 0.226 | -1.547 | -0.246 | â |
| Soubiran et al. | 2018 | 14.34 | 62.125 | â | â | â | -80.22 |
| Bica et al. | 2019 | 14.309 | 62.104 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 14.34 | 62.125 | 0.226 | -1.547 | -0.246 | â |
| Kharchenko et al. | 2016 | 14.31 | 62.122 | â | â | â | â |
| Kharchenko et al. | 2013 | 14.32 | 62.125 | â | -1.57 | -0.07 | â |
| Kharchenko et al. | 2012 | 14.32 | 62.125 | â | -1.57 | -0.07 | â |
| Glushkova et al. | 2010 | 14.302 | 62.105 | â | â | â | â |
| Froebrich et al. | 2007 | 14.338 | 62.114 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.59 | 2.99 | â | 274 | â | 210 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 936* | â | â |
| Cavallo et al. | 2024 | 3.21 | 3.82 | â | 282 | -0.480 | â | â | â |
| Hunt & Reffert | 2023 | 3.69 | 3.34 | 1.96 | 220 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1549 | â | 91 | â | â |
| Dias et al. | 2021 | 3.59 | 2.99 | â | 274 | 0.168 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.91 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.91 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.91 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.84 | 1.68 | â | 1549 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.84 | 1.68 | â | 1549 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.84 | 1.68 | â | 1549 | â | â | â | â |
| Glushkova et al. | 2010 | 1.38 | 1.58 | â | 1259 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.