FSR 1521
(SAI 111; MWSC 1727)
0.85
UTI
0.87
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
3.1 [arcmin]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1521 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
Distant
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 148.85 | -56.608 | 0.235 | -4.762 | 4.72 | 52.392 |
| Almeida et al. | 2025 | 148.846 | -56.601 | â | â | â | â |
| Hunt & Reffert | 2024 | 148.83 | -56.617 | 0.251 | -4.696 | 4.799 | 49.744 |
| Cavallo et al. | 2024 | 148.844 | -56.592 | 0.237 | â | â | â |
| Hunt & Reffert | 2023 | 148.83 | -56.617 | 0.251 | -4.696 | 4.799 | 49.744 |
| Just et al. | 2023 | 148.824 | -56.611 | â | â | â | â |
| Dias et al. | 2021 | 148.846 | -56.601 | 0.189 | -4.8 | 4.595 | â |
| Cantat-Gaudin et al. | 2020 | 148.852 | -56.605 | 0.201 | -4.886 | 4.467 | â |
| Cantat-Gaudin & Anders | 2020 | 148.852 | -56.605 | 0.201 | -4.886 | 4.467 | â |
| Soubiran et al. | 2018 | 148.852 | -56.605 | â | â | â | 55.54 |
| Bica et al. | 2019 | 148.847 | -56.608 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 148.852 | -56.605 | 0.201 | -4.886 | 4.467 | â |
| Kharchenko et al. | 2016 | 148.824 | -56.611 | â | â | â | â |
| Kharchenko et al. | 2013 | 148.83 | -56.615 | â | -8.92 | 6.1 | â |
| Glushkova et al. | 2010 | 148.844 | -56.604 | â | â | â | â |
| Froebrich et al. | 2007 | 148.846 | -56.602 | 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 | 6.54 | 3.20 | â | 1271 | â | 2133 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3412* | â | â |
| Cavallo et al. | 2024 | 5.78 | 3.04 | â | 1175 | -0.230 | â | â | â |
| Hunt & Reffert | 2023 | 3.61 | 3.54 | 2.94 | 1507 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 507 | â | 102 | â | â |
| Dias et al. | 2021 | 6.54 | 3.20 | â | 1271 | 0.178 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.94 | 2.72 | â | 5248 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.34 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.34 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.34 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.50 | 1.16 | â | 507 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.50 | 1.16 | â | 507 | â | â | â | â |
| Glushkova et al. | 2010 | 3.98 | 2.79 | â | 2818 | 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)
Bronze sample.