FoF 1375
0.36
UTI
0.43
CN
0.32
Cdens
0.38
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
1.6 [N/pc2]
- CN 0.43 Poorly populated
- Cdens 0.32 Loose
- CC3 0.38 Low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
FoF 1375 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 91.036 | 28.046 | 0.218 | 0.385 | -1.086 | 33.919 |
| Hu & Soubiran | 2025 | 91.052 | 28.054 | â | â | â | â |
| Zhang et al. | 2024 | 91.038 | 28.047 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.038 | 28.047 | 0.207 | 0.402 | -1.012 | 28.661 |
| Cavallo et al. | 2024 | 91.052 | 28.054 | 0.205 | â | â | â |
| Hunt & Reffert | 2023 | 91.038 | 28.047 | 0.207 | 0.402 | -1.012 | 28.661 |
| Liu & Pang | 2019 | 91.042 | 28.045 | 0.259 | 0.264 | -1.593 | 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 | 4.02 | 0.56 | 1.67 | 562 | -0.165 | 532 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.305(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 532(1) | â | â |
| Cavallo et al. | 2024 | 3.55 | 0.57 | â | 851 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 4.49 | 0.55 | 1.67 | 507 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 562 | 0.500 | 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.