FoF 2383
(OCSN 209)
0.74
UTI
0.89
CN
1.0
Cdens
1.0
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
27.7 [N/pc2]
- CN 0.89 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
FoF 2383 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 95.329 | -16.136 | 2.695 | -5.393 | 5.028 | 23.211 |
| Wei et al. | 2025 | 95.353 | -16.215 | 2.717 | -5.384 | 5.014 | â |
| Hunt & Reffert | 2024 | 95.38 | -16.097 | 2.692 | -5.37 | 5.049 | 22.239 |
| Cavallo et al. | 2024 | 95.249 | -16.297 | 2.695 | â | â | â |
| Hunt & Reffert | 2023 | 95.38 | -16.097 | 2.692 | -5.37 | 5.049 | 22.239 |
| Qin et al. | 2023 | 95.35 | -16.1 | 2.81 | -5.44 | 5.13 | 23.37 |
| He et al. | 2022 | 95.21 | -16.215 | 2.712 | -5.25 | 5.081 | â |
| Liu & Pang | 2019 | 95.383 | -16.044 | 2.651 | -5.377 | 4.967 | 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 | 0.39 | 0.42 | 0.64 | 34 | 0.250 | 291 | 0.39 | â |
| Wei et al. | 2025 | 0.44 | 0.42 | â | 33 | 0.250 | 368 | 0.39 | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 214(1) | â | â |
| Cavallo et al. | 2024 | 0.38 | 0.54 | â | 14 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 0.36 | 0.15 | 0.64 | 38 | â | â | â | â |
| Qin et al. | 2023 | 0.40 | 0.31 | â | 40 | â | â | â | â |
| He et al. | 2022 | â | 0.45 | â | 35 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 33 | 0.250 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P254, along with HSC_1751.
Cavallo et al. (2024)
Gold sample.