FoF 597
(LP 597)
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 597 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 moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age 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
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 282.104 | 8.715 | 0.432 | -0.06 | -1.475 | 26.303 |
| Li et al. | 2025 | 282.104 | 8.714 | 0.418 | -0.058 | -1.49 | â |
| Almeida et al. | 2025 | 282.099 | 8.717 | â | â | â | â |
| Zhang et al. | 2024 | 282.114 | 8.709 | â | â | â | â |
| Hunt & Reffert | 2024 | 282.114 | 8.709 | 0.439 | -0.089 | -1.493 | 43.712 |
| Cavallo et al. | 2024 | 282.1 | 8.711 | 0.437 | â | â | â |
| Hunt & Reffert | 2023 | 282.114 | 8.709 | 0.439 | -0.089 | -1.493 | 43.712 |
| Almeida et al. | 2023 | 282.103 | 8.725 | â | â | â | â |
| Dias et al. | 2021 | 282.099 | 8.717 | 0.412 | -0.062 | -1.486 | 25.139 |
| Cantat-Gaudin et al. | 2020 | 282.104 | 8.714 | 0.418 | -0.058 | -1.49 | â |
| Liu & Pang | 2019 | 282.108 | 8.727 | 0.434 | -0.075 | -1.46 | 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 | 2.08 | 2.98 | â | 839 | 0.232 | â | â | â |
| Almeida et al. | 2025 | 2.06 | 3.00 | â | 568 | â | 706 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.150* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1998* | â | â |
| Cavallo et al. | 2024 | 2.26 | 3.38 | â | 316 | 0.460 | â | â | â |
| Hunt & Reffert | 2023 | 2.14 | 3.14 | 1.27 | 269 | â | â | â | â |
| Almeida et al. | 2023 | 2.00 | 2.94 | â | 624 | 0.119 | 1099* | 0.69 | â |
| Dias et al. | 2021 | 2.06 | 3.00 | â | 568 | 0.075 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.09 | 2.46 | â | 537 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1780 | -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: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.