FoF 145
(LP 145)
0.76
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
46.1 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
FoF 145 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a very 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 contains blue stragglers according to at least one source.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 256.987 | -44.152 | 0.531 | -2.122 | -5.478 | -9.823 |
| Hu & Soubiran | 2025 | 256.968 | -44.166 | â | â | â | â |
| Carrasco-Varela et al. | 2025 | 256.957 | -44.157 | â | â | â | â |
| Almeida et al. | 2025 | 256.957 | -44.157 | â | â | â | â |
| Hunt & Reffert | 2024 | 256.986 | -44.156 | 0.532 | -2.114 | -5.5 | -4.148 |
| Cavallo et al. | 2024 | 256.968 | -44.166 | 0.533 | â | â | â |
| Hunt & Reffert | 2023 | 256.986 | -44.156 | 0.532 | -2.114 | -5.5 | -4.148 |
| Dias et al. | 2021 | 256.957 | -44.157 | 0.526 | -2.116 | -5.419 | -11.264 |
| Cantat-Gaudin et al. | 2020 | 256.976 | -44.157 | 0.521 | -2.091 | -5.424 | â |
| Liu & Pang | 2019 | 256.981 | -44.132 | 0.518 | -2.103 | -5.424 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.81 | 3.82 | 2.71 | 714 | 0.250 | 5722 | â | 0.06 |
| Hu & Soubiran | 2025 | â | â | â | â | -0.100(5) | â | â | â |
| Carrasco-Varela et al. | 2025 | 1.81 | 3.92 | â | 714 | 0.400 | â | â | 0.06(1) |
| Almeida et al. | 2025 | 1.81 | 3.72 | â | 714 | â | 2944 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 8499(1) | â | â |
| Cavallo et al. | 2024 | 1.61 | 4.32 | â | 617 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.74 | 4.67 | 2.71 | 281 | â | â | â | â |
| Dias et al. | 2021 | 1.81 | 3.72 | â | 714 | 0.073 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.99 | 3.00 | â | 1000 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 977 | 0.250 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.