Gulliver 54
0.70
UTI
0.55
CN
1.0
Cdens
0.38
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
7.4 [arcmin]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 54 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.
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 | 81.261 | 33.693 | 0.813 | -0.509 | -7.22 | 14.053 |
| Li et al. | 2025 | 81.297 | 33.688 | 0.791 | -0.595 | -7.299 | â |
| Almeida et al. | 2025 | 81.271 | 33.696 | â | â | â | â |
| Zhang et al. | 2024 | 81.272 | 33.678 | â | â | â | â |
| Hunt & Reffert | 2024 | 81.272 | 33.678 | 0.82 | -0.507 | -7.265 | 6.031 |
| Cavallo et al. | 2024 | 81.278 | 33.706 | 0.822 | â | â | â |
| Hunt & Reffert | 2023 | 81.272 | 33.678 | 0.82 | -0.507 | -7.265 | 6.031 |
| He et al. | 2022 | 81.251 | 33.703 | 0.832 | -0.478 | -7.223 | â |
| Tarricq et al. | 2022 | 81.247 | 33.69 | 0.841 | -0.506 | -7.248 | â |
| Dias et al. | 2021 | 81.271 | 33.696 | 0.777 | -0.605 | -7.245 | â |
| Cantat-Gaudin et al. | 2020 | 81.297 | 33.688 | 0.791 | -0.595 | -7.299 | â |
| Cantat-Gaudin & Anders | 2020 | 81.297 | 33.688 | 0.791 | -0.595 | -7.299 | â |
| Monteiro & Dias | 2019 | 81.297 | 33.688 | â | â | â | 2.951 |
| Soubiran et al. | 2018 | 81.297 | 33.688 | â | â | â | 16.77 |
| Cantat-Gaudin et al. | 2018 | 81.297 | 33.688 | 0.791 | -0.595 | -7.299 | 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 | 1.13 | 0.66 | â | 422 | -0.047 | â | â | â |
| Almeida et al. | 2025 | 1.21 | 0.88 | â | 253 | â | 103 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.192* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 175* | â | â |
| Cavallo et al. | 2024 | 1.14 | 0.71 | â | 347 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 1.19 | 0.70 | 1.15 | 369 | â | â | â | â |
| He et al. | 2022 | â | 0.70 | â | 355 | â | â | â | â |
| Tarricq et al. | 2022 | 1.15 | â | â | 302 | â | â | â | â |
| Dias et al. | 2021 | 1.21 | 0.88 | â | 253 | -0.151 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.19 | 0.40 | â | 282 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.22 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.19 | 0.52 | â | 419 | 0.017 | â | â | â |
| Soubiran et al. | 2018 | 1.22 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.22 | 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.