FoF 1825
(LP 1825)
0.15
UTI
0.37
CN
0.14
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
6.3 [arcmin]
- CN 0.37 Poorly populated
- Cdens 0.14 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 1825 is a poorly populated, 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 massive, near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.97 kpc) differs significantly from the median photometric distance (~2.92 kpc).
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.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 359.163 | 62.894 | 0.252 | -2.632 | -0.954 | â |
| Almeida et al. | 2025 | 359.229 | 62.878 | â | â | â | â |
| Dias et al. | 2021 | 359.229 | 62.878 | 0.267 | -2.667 | -0.921 | -52.56 |
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 | 2.92 | 1.80 | â | 27 | â | 2659 | â | â |
| Dias et al. | 2021 | 2.92 | 1.80 | â | 27 | -0.062 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.