FoF 1429
(LP 1429)
0.41
UTI
0.81
CN
0.59
Cdens
0.75
CC3
0.0
Clit
0.94
Cdup
Stellar density (N50/rad)
2.9 [N/pc2]
- CN 0.81 Rich
- Cdens 0.59 Moderately dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.94 Very likely 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 1429 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a moderate* distance, near 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.
(*): The parallax distance estimate (~4.72 kpc) differs significantly from the median photometric distance (~3.47 kpc).
Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 119.419 | -28.542 | 0.212 | -2.307 | 2.892 | 76.796 |
| Almeida et al. | 2025 | 119.398 | -28.542 | â | â | â | â |
| Dias et al. | 2021 | 119.398 | -28.542 | 0.246 | -2.308 | 2.866 | 78.594 |
| Liu & Pang | 2019 | 119.362 | -28.537 | 0.254 | -2.263 | 2.814 | 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 | 3.47 | 1.24 | â | 175 | 0.229 | 1064 | â | â |
| Almeida et al. | 2025 | 3.47 | 1.24 | â | 175 | â | 1064 | â | â |
| Dias et al. | 2021 | 3.47 | 1.24 | â | 175 | -0.042 | â | â | â |
| Liu & Pang | 2019 | â | â | â | 501 | 0.500 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.