Gulliver 60
(FoF 2124)
0.85
UTI
0.85
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
10.7 [arcmin]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 60 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 303.441 | 29.683 | 0.905 | 1.724 | 0.161 | -11.391 |
| Li et al. | 2025 | 303.436 | 29.672 | 0.899 | 1.752 | 0.219 | â |
| Almeida et al. | 2025 | 303.443 | 29.69 | â | â | â | â |
| Zhang et al. | 2024 | 303.445 | 29.66 | â | â | â | â |
| Hunt & Reffert | 2024 | 303.445 | 29.66 | 0.922 | 1.739 | 0.15 | -11.113 |
| Cavallo et al. | 2024 | 303.421 | 29.685 | 0.918 | â | â | â |
| Hunt & Reffert | 2023 | 303.445 | 29.66 | 0.922 | 1.739 | 0.15 | -11.113 |
| Almeida et al. | 2023 | 303.452 | 29.707 | â | â | â | â |
| He et al. | 2022 | 303.456 | 29.668 | 0.906 | 1.74 | 0.16 | â |
| Tarricq et al. | 2022 | 303.432 | 29.655 | 0.899 | 1.751 | 0.171 | â |
| Dias et al. | 2021 | 303.443 | 29.69 | 0.9 | 1.75 | 0.222 | â |
| Cantat-Gaudin et al. | 2020 | 303.436 | 29.672 | 0.899 | 1.752 | 0.219 | â |
| Cantat-Gaudin & Anders | 2020 | 303.436 | 29.672 | 0.899 | 1.752 | 0.219 | â |
| Liu & Pang | 2019 | 303.448 | 29.684 | 0.909 | 1.752 | 0.191 | â |
| Monteiro & Dias | 2019 | 303.436 | 29.672 | â | â | â | 2.613 |
| Cantat-Gaudin et al. | 2018 | 303.436 | 29.672 | 0.899 | 1.752 | 0.219 | 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 | 1.03 | 1.11 | â | 85 | 0.157 | â | â | â |
| Almeida et al. | 2025 | 1.07 | 1.50 | â | 91 | â | 393 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.188* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 811* | â | â |
| Cavallo et al. | 2024 | 1.16 | 1.43 | â | 72 | 0.450 | â | â | â |
| Hunt & Reffert | 2023 | 1.05 | 1.43 | 1.77 | 84 | â | â | â | â |
| Almeida et al. | 2023 | 1.05 | 1.36 | â | 98 | 0.184 | 347* | 0.56 | â |
| He et al. | 2022 | â | 1.60 | â | 40 | â | â | â | â |
| Tarricq et al. | 2022 | 1.04 | â | â | 95 | â | â | â | â |
| Dias et al. | 2021 | 1.07 | 1.50 | â | 91 | -0.031 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.06 | 1.01 | â | 93 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.08 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 44 | -0.250 | â | â | â |
| Monteiro & Dias | 2019 | 1.22 | 1.17 | â | 136 | 0.038 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.08 | â | â | â | â | 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.