FoF 1437
(LP 1437)
0.12
UTI
0.32
CN
0.16
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
4.6 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.16 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 1437 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
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.
Distant
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 124.12 | -33.637 | 0.212 | -2.615 | 3.043 | 76.945 |
| Almeida et al. | 2025 | 124.106 | -33.662 | â | â | â | â |
| Dias et al. | 2021 | 124.106 | -33.662 | 0.237 | -2.601 | 3.041 | 64.672 |
| Liu & Pang | 2019 | 124.115 | -33.669 | 0.246 | -2.591 | 3.033 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.63 | 1.13 | â | 322 | â | 4534 | â | â |
| Dias et al. | 2021 | 3.63 | 1.13 | â | 322 | -0.136 | â | â | â |
| Liu & Pang | 2019 | â | â | â | 525 | 0.500 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.