FoF 1428
0.17
UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
0.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.25 Low quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
FoF 1428 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 119.412 | -28.028 | 0.306 | -2.638 | 2.705 | 62.268 |
| Hunt & Reffert | 2024 | 119.271 | -27.915 | 0.304 | -2.955 | 2.807 | â |
| Cavallo et al. | 2024 | 119.272 | -27.883 | 0.303 | â | â | â |
| Hunt & Reffert | 2023 | 119.271 | -27.915 | 0.304 | -2.955 | 2.807 | â |
| Liu & Pang | 2019 | 119.397 | -28.067 | 0.279 | -2.388 | 2.551 | 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 | 2.79 | 1.08 | 1.84 | 103 | 0.160 | 273 | â | â |
| Liu et al. | 2025 | 3.66 | 0.30 | â | 95 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 273(1) | â | â |
| Cavallo et al. | 2024 | 2.73 | 1.18 | â | 87 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 2.79 | 1.08 | 1.84 | 111 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 692 | 0.250 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Dias et al. (2021)
Dubious open cluster.
Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 115 along with CWNU_2312.
Palma et al. (2025)
Classified as optical pair P109, along with CWNU_2312.
Cavallo et al. (2024)
Gold sample.