FoF 2309
0.60
UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
17.8 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
FoF 2309 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near 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 large percentage of members with a later reported entry. 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 | 209.929 | -63.605 | 1.03 | -6.157 | -1.715 | 9.608 |
| Hu & Soubiran | 2025 | 209.914 | -63.611 | â | â | â | â |
| Hunt & Reffert | 2024 | 209.963 | -63.611 | 1.024 | -6.189 | -1.722 | 9.394 |
| Cavallo et al. | 2024 | 209.914 | -63.611 | 1.028 | â | â | â |
| Hunt & Reffert | 2023 | 209.963 | -63.611 | 1.024 | -6.189 | -1.722 | 9.394 |
| He et al. | 2022 | 209.924 | -63.623 | 1.033 | -6.169 | -1.683 | â |
| Liu & Pang | 2019 | 209.942 | -63.613 | 1.0 | -6.165 | -1.758 | 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 | 0.955 | 0.81 | 0.28 | 669 | -0.060 | 215 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.060(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 215(1) | â | â |
| Cavallo et al. | 2024 | 0.99 | 0.71 | â | 891 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 0.92 | 0.81 | 0.28 | 352 | â | â | â | â |
| He et al. | 2022 | â | 1.25 | â | 447 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1150 | -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.