FSR 0975
0.76
UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
5.5 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0975 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 | 100.007 | 13.313 | 0.182 | 0.171 | -0.822 | 63.263 |
| Hu & Soubiran | 2025 | 100.004 | 13.317 | â | â | â | â |
| Zhang et al. | 2024 | 100.006 | 13.311 | â | â | â | â |
| Hunt & Reffert | 2024 | 100.006 | 13.311 | 0.18 | 0.163 | -0.798 | 35.367 |
| Cavallo et al. | 2024 | 100.004 | 13.317 | 0.182 | â | â | â |
| Hunt & Reffert | 2023 | 100.006 | 13.311 | 0.18 | 0.163 | -0.798 | 35.367 |
| Cantat-Gaudin et al. | 2020 | 100.01 | 13.31 | 0.173 | 0.166 | -0.817 | â |
| Zhong et al. | 2020 | 100.01 | 13.31 | â | 0.166 | -0.817 | 35.1 |
| Cantat-Gaudin & Anders | 2020 | 100.01 | 13.31 | 0.173 | 0.166 | -0.817 | â |
| Bica et al. | 2019 | 100.001 | 13.304 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 100.01 | 13.31 | 0.173 | 0.166 | -0.817 | â |
| Dias et al. | 2014 | 100.0 | 13.299 | â | 2.11 | 2.86 | â |
| Froebrich et al. | 2007 | 100.0 | 13.299 | â | â | â | â |
| Dias et al. | 2002 | 100.0 | 13.299 | â | 2.11 | 2.86 | 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 | 4.61 | 0.9 | 1.89 | 627 | -0.100 | 559 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.200(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.302(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 559(1) | â | â |
| Cavallo et al. | 2024 | 4.51 | 0.72 | â | 692 | 0.570 | â | â | â |
| Hunt & Reffert | 2023 | 4.59 | 1.08 | 1.89 | 562 | â | â | â | â |
| Zhong et al. | 2020 | 0.00 | 0.00 | â | 0 | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.96 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.96 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 4.63 | 1.68 | â | 1259 | 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.