FoF 1160
(LP 1160)
0.05
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
10.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 1160 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.
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
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 201.969 | -63.449 | 0.231 | -6.834 | -1.399 | -24.428 |
| Almeida et al. | 2025 | 202.096 | -63.477 | â | â | â | â |
| Dias et al. | 2021 | 202.096 | -63.477 | 0.257 | -6.829 | -1.396 | 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 | 3.56 | 2.13 | â | 12 | â | 1484 | â | â |
| Dias et al. | 2021 | 3.56 | 2.13 | â | 12 | 0.048 | â | â | â |
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.