FSR 1452
(MWSC 1597; FoF 107)
0.80
UTI
0.83
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
18.7 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1452 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, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, 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 | 133.319 | -47.867 | 0.384 | -4.596 | 3.789 | 20.4 |
| Li et al. | 2025 | 133.332 | -47.871 | 0.363 | -4.603 | 3.722 | â |
| Hunt & Reffert | 2024 | 133.328 | -47.855 | 0.387 | -4.601 | 3.833 | 20.307 |
| Cavallo et al. | 2024 | 133.27 | -47.828 | 0.386 | â | â | â |
| Hunt & Reffert | 2023 | 133.328 | -47.855 | 0.387 | -4.601 | 3.833 | 20.307 |
| Just et al. | 2023 | 133.322 | -47.917 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 133.332 | -47.871 | 0.363 | -4.603 | 3.722 | â |
| Cantat-Gaudin & Anders | 2020 | 133.332 | -47.871 | 0.363 | -4.603 | 3.722 | â |
| Liu & Pang | 2019 | 133.319 | -47.862 | 0.377 | -4.566 | 3.812 | â |
| Soubiran et al. | 2018 | 133.332 | -47.871 | â | â | â | 16.23 |
| Cantat-Gaudin et al. | 2018 | 133.332 | -47.871 | 0.363 | -4.603 | 3.722 | â |
| Kharchenko et al. | 2016 | 133.322 | -47.917 | â | â | â | â |
| Kharchenko et al. | 2013 | 133.327 | -47.92 | â | -2.74 | 10.15 | â |
| Froebrich et al. | 2007 | 133.283 | -47.92 | 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 | 2.33 | 1.735 | 2.62 | 606 | -0.043 | 1024 | â | â |
| Li et al. | 2025 | 2.22 | 2.01 | â | 224 | -0.043 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1920(1) | â | â |
| Cavallo et al. | 2024 | 2.49 | 2.33 | â | 148 | 0.310 | â | â | â |
| Hunt & Reffert | 2023 | 2.33 | 1.98 | 2.62 | 164 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1122 | â | 129 | â | â |
| Cantat-Gaudin et al. | 2020 | 2.30 | 1.49 | â | 234 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.55 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 977 | -2.000 | â | â | â |
| Soubiran et al. | 2018 | 2.55 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.55 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.07 | 1.16 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.07 | 1.16 | â | 1122 | 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)
Gold sample.