Gulliver 56
0.80
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 56 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
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 | 95.383 | 26.924 | 0.439 | 0.444 | -3.195 | 31.754 |
| Li et al. | 2025 | 95.38 | 26.909 | 0.458 | 0.534 | -3.24 | â |
| Hu & Soubiran | 2025 | 95.387 | 26.94 | â | â | â | â |
| Almeida et al. | 2025 | 95.389 | 26.928 | â | â | â | â |
| Zhang et al. | 2024 | 95.392 | 26.901 | â | â | â | â |
| Hunt & Reffert | 2024 | 95.392 | 26.901 | 0.428 | 0.426 | -3.185 | 70.304 |
| Cavallo et al. | 2024 | 95.387 | 26.94 | 0.431 | â | â | â |
| Hunt & Reffert | 2023 | 95.392 | 26.901 | 0.428 | 0.426 | -3.185 | 70.304 |
| Almeida et al. | 2023 | 95.389 | 26.924 | â | â | â | â |
| Dias et al. | 2021 | 95.389 | 26.928 | 0.459 | 0.545 | -3.247 | â |
| Cantat-Gaudin et al. | 2020 | 95.38 | 26.909 | 0.458 | 0.534 | -3.24 | â |
| Cantat-Gaudin & Anders | 2020 | 95.38 | 26.909 | 0.458 | 0.534 | -3.24 | â |
| Monteiro & Dias | 2019 | 95.38 | 26.909 | â | â | â | 2.246 |
| Cantat-Gaudin et al. | 2018 | 95.38 | 26.909 | 0.458 | 0.534 | -3.24 | 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 | 1.93 | 0.85 | â | 416 | -0.135 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.130* | â | â | â |
| Almeida et al. | 2025 | 1.94 | 0.97 | â | 224 | â | 163 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.156* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 614* | â | â |
| Cavallo et al. | 2024 | 2.07 | 0.64 | â | 661 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 2.05 | 0.38 | 1.05 | 618 | â | â | â | â |
| Almeida et al. | 2023 | 1.96 | 0.90 | â | 331 | -0.084 | 269* | 0.53 | â |
| Dias et al. | 2021 | 1.94 | 0.97 | â | 224 | -0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.07 | 0.44 | â | 407 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.05 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 2.61 | 1.03 | â | 223 | 0.029 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.05 | 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.
Cavallo et al. (2024)
Gold sample.