FoF 2249
(LP 2249)
0.40
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.67
Cdup
Radius (P>50% members)
17.6 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.0 Rarely studied
- Cdup 0.67 Likely unique
Overview
FoF 2249 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a close 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 is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.
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 | 344.272 | 62.761 | 1.179 | -0.949 | -2.285 | -19.964 |
| Almeida et al. | 2025 | 344.815 | 62.843 | â | â | â | â |
| Dias et al. | 2021 | 344.815 | 62.843 | 1.159 | -1.059 | -2.248 | -26.631 |
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 | 0.82 | 2.19 | â | 5 | â | 2198 | â | â |
| Dias et al. | 2021 | 0.82 | 2.19 | â | 5 | -0.031 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.