Gulliver 25
0.67
UTI
0.57
CN
0.65
Cdens
0.62
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
11.3 [arcmin]
- CN 0.57 Moderately populated
- Cdens 0.65 Moderately dense
- CC3 0.62 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 25 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Relatively close
Low extinction
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 | 52.0 | 45.166 | 0.736 | 0.917 | -4.163 | -30.762 |
| Li et al. | 2025 | 52.011 | 45.152 | 0.711 | 0.96 | -4.089 | â |
| Almeida et al. | 2025 | 52.067 | 45.132 | â | â | â | â |
| Zhang et al. | 2024 | 51.995 | 45.179 | â | â | â | â |
| Hunt & Reffert | 2024 | 51.995 | 45.179 | 0.738 | 0.914 | -4.203 | -22.598 |
| Cavallo et al. | 2024 | 52.641 | 44.879 | 0.735 | â | â | â |
| Hunt & Reffert | 2023 | 51.995 | 45.179 | 0.738 | 0.914 | -4.203 | -22.598 |
| Almeida et al. | 2023 | 52.1 | 45.143 | â | â | â | â |
| Tarricq et al. | 2022 | 51.983 | 45.213 | 0.742 | 0.909 | -4.149 | â |
| Dias et al. | 2021 | 52.067 | 45.132 | 0.702 | 0.962 | -4.075 | â |
| Cantat-Gaudin et al. | 2020 | 52.011 | 45.152 | 0.711 | 0.96 | -4.089 | â |
| Cantat-Gaudin & Anders | 2020 | 52.011 | 45.152 | 0.711 | 0.96 | -4.089 | â |
| Monteiro & Dias | 2019 | 52.011 | 45.152 | â | â | â | 3.125 |
| Cantat-Gaudin et al. | 2018 | 52.011 | 45.152 | 0.711 | 0.96 | -4.089 | 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 | 1.55 | 0.90 | â | 348 | 0.246 | â | â | â |
| Almeida et al. | 2025 | 1.27 | 0.99 | â | 458 | â | 112 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.242* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 89* | â | â |
| Cavallo et al. | 2024 | 1.32 | 1.21 | â | 269 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 1.27 | 0.81 | 0.39 | 191 | â | â | â | â |
| Almeida et al. | 2023 | 1.29 | 1.07 | â | 296 | -0.110 | 258* | 0.50 | â |
| Tarricq et al. | 2022 | 1.31 | â | â | 363 | â | â | â | â |
| Dias et al. | 2021 | 1.27 | 0.99 | â | 458 | -0.029 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.36 | 0.82 | â | 363 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.35 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.32 | 0.75 | â | 365 | 0.024 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.35 | 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.