Gulliver 45
0.72
UTI
0.68
CN
1.0
Cdens
0.62
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
2.9 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 45 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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.
Distant
Moderate 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 | 104.617 | 3.093 | 0.294 | -0.748 | 2.448 | 28.391 |
| Hu & Soubiran | 2025 | 104.605 | 3.125 | â | â | â | â |
| Almeida et al. | 2025 | 104.608 | 3.111 | â | â | â | â |
| Hunt & Reffert | 2024 | 104.621 | 3.09 | 0.296 | -0.753 | 2.437 | â |
| Cavallo et al. | 2024 | 104.605 | 3.125 | 0.286 | â | â | â |
| Hunt & Reffert | 2023 | 104.621 | 3.09 | 0.296 | -0.753 | 2.437 | â |
| Dias et al. | 2021 | 104.608 | 3.111 | 0.289 | -0.793 | 2.474 | â |
| Cantat-Gaudin et al. | 2020 | 104.617 | 3.104 | 0.284 | -0.76 | 2.51 | â |
| Cantat-Gaudin & Anders | 2020 | 104.617 | 3.104 | 0.284 | -0.76 | 2.51 | â |
| Monteiro & Dias | 2019 | 104.617 | 3.104 | â | â | â | 2.772 |
| Soubiran et al. | 2018 | 104.617 | 3.104 | â | â | â | 135.26 |
| Cantat-Gaudin et al. | 2018 | 104.617 | 3.104 | 0.284 | -0.76 | 2.51 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.170* | â | â | â |
| Almeida et al. | 2025 | 3.17 | 1.38 | â | 4083 | â | 403 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 529* | â | â |
| Cavallo et al. | 2024 | 3.21 | 1.21 | â | 3162 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 3.21 | 1.10 | 1.09 | 3069 | â | â | â | â |
| Dias et al. | 2021 | 3.17 | 1.38 | â | 4083 | -0.103 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.33 | 1.08 | â | 3090 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.20 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 3.39 | 1.14 | â | 4093 | 0.023 | â | â | â |
| Soubiran et al. | 2018 | 3.20 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.20 | 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: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.