FoF 2113
(LP 2113)
0.13
UTI
0.0
CN
0.29
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.29 Loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
FoF 2113 is a sparse, 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 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.
Relatively close
Moderate extinction
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 | 274.712 | -18.09 | 0.433 | -0.267 | -1.98 | -25.781 |
| Almeida et al. | 2025 | 274.705 | -18.078 | â | â | â | â |
| Dias et al. | 2021 | 274.705 | -18.078 | 0.475 | -0.309 | -1.976 | 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 | 2.01 | 1.59 | â | 15 | â | 346 | â | â |
| Dias et al. | 2021 | 2.01 | 1.59 | â | 15 | 0.135 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.