FoF 1692
(LP 1692)
0.42
UTI
0.35
CN
0.98
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
2.0 [arcmin]
- CN 0.35 Poorly populated
- Cdens 0.98 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 1692 is a poorly populated, very dense object of high 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, very young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Distant
Moderate extinction
Massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 289.178 | 14.153 | 0.218 | -2.148 | -5.452 | 58.432 |
| Almeida et al. | 2025 | 289.171 | 14.156 | â | â | â | â |
| He et al. | 2023 | 289.182 | 14.164 | 0.204 | -2.156 | -5.51 | 58.43 |
| Dias et al. | 2021 | 289.171 | 14.156 | 0.244 | -2.169 | -5.371 | 31.952 |
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 | 3.93 | 2.91 | â | 8 | â | 1579 | â | â |
| He et al. | 2023 | 3.72 | 3.50 | â | 10 | â | â | â | â |
| Dias et al. | 2021 | 3.93 | 2.91 | â | 8 | 0.269 | â | â | â |
Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.