FoF 1540
(LP 1540)
0.79
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
3.3 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
FoF 1540 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 170.231 | -59.295 | 0.35 | -5.24 | 1.817 | -22.796 |
| Li et al. | 2025 | 170.219 | -59.302 | 0.346 | -5.245 | 1.807 | â |
| Hu & Soubiran | 2025 | 170.212 | -59.291 | â | â | â | â |
| Almeida et al. | 2025 | 170.226 | -59.302 | â | â | â | â |
| Hunt & Reffert | 2024 | 170.212 | -59.301 | 0.341 | -5.261 | 1.808 | -20.544 |
| Cavallo et al. | 2024 | 170.212 | -59.291 | 0.346 | â | â | â |
| Hunt & Reffert | 2023 | 170.212 | -59.301 | 0.341 | -5.261 | 1.808 | -20.544 |
| Almeida et al. | 2023 | 170.231 | -59.306 | â | â | â | â |
| Dias et al. | 2021 | 170.226 | -59.302 | 0.353 | -5.245 | 1.811 | 24.983 |
| Cantat-Gaudin et al. | 2020 | 170.219 | -59.302 | 0.346 | -5.245 | 1.807 | â |
| Liu & Pang | 2019 | 170.199 | -59.306 | 0.337 | -5.341 | 1.801 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.57 | 0.88 | â | 1536 | -0.228 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.290* | â | â | â |
| Almeida et al. | 2025 | 2.37 | 0.81 | â | 1387 | â | 301 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 649* | â | â |
| Cavallo et al. | 2024 | 2.23 | 0.81 | â | 1413 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 2.65 | 0.55 | 0.48 | 1052 | â | â | â | â |
| Almeida et al. | 2023 | 2.45 | 0.81 | â | 1449 | -0.008 | 934* | 0.64 | â |
| Dias et al. | 2021 | 2.37 | 0.81 | â | 1387 | -0.090 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.54 | 0.49 | â | 1622 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1020 | 0.500 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.