FoF 1352
(LP 1352)
0.08
UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
14.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 1352 is a sparse, very loose object of low 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, very young cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.24 kpc) differs significantly from the median photometric distance (~2.39 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
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 29.482 | 60.458 | 0.309 | -1.01 | -0.387 | â |
| Almeida et al. | 2025 | 29.3 | 60.514 | â | â | â | â |
| Dias et al. | 2021 | 29.3 | 60.514 | 0.289 | -1.006 | -0.362 | -73.739 |
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 | 2.39 | 2.39 | â | 19 | â | 1299 | â | â |
| Dias et al. | 2021 | 2.39 | 2.39 | â | 19 | -0.217 | â | â | â |
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.