FoF 1414
(LP 1414)
0.13
UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
4.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 1414 is a sparse, very loose object of intermediate 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, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.
Note: This object shares a significant 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
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 116.441 | -19.167 | 0.243 | -1.723 | 2.244 | â |
| Almeida et al. | 2025 | 116.418 | -19.138 | â | â | â | â |
| He et al. | 2023 | 116.41 | -19.181 | 0.237 | -1.677 | 2.199 | â |
| Dias et al. | 2021 | 116.418 | -19.138 | 0.251 | -1.841 | 2.264 | 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 | 3.44 | 1.22 | â | 87 | â | 1245 | â | â |
| He et al. | 2023 | 3.47 | 0.75 | â | 501 | â | â | â | â |
| Dias et al. | 2021 | 3.44 | 1.22 | â | 87 | -0.101 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.