Gulliver 12
(FoF 2152)
0.80
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 12 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 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 large percentage of members with a later reported entry. 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 | 181.187 | -61.313 | 0.573 | -5.962 | -0.377 | 6.873 |
| Li et al. | 2025 | 181.174 | -61.308 | 0.559 | -5.948 | -0.41 | â |
| Almeida et al. | 2025 | 181.192 | -61.31 | â | â | â | â |
| Hunt & Reffert | 2024 | 181.17 | -61.312 | 0.581 | -5.943 | -0.373 | -8.07 |
| Cavallo et al. | 2024 | 181.242 | -61.335 | 0.582 | â | â | â |
| Hunt & Reffert | 2023 | 181.17 | -61.312 | 0.581 | -5.943 | -0.373 | -8.07 |
| Almeida et al. | 2023 | 181.209 | -61.33 | â | â | â | â |
| Rain et al. | 2021 | 181.174 | -61.308 | 0.559 | -5.948 | -0.41 | â |
| Dias et al. | 2021 | 181.192 | -61.31 | 0.559 | -5.947 | -0.421 | â |
| Cantat-Gaudin et al. | 2020 | 181.174 | -61.308 | 0.559 | -5.948 | -0.41 | â |
| Cantat-Gaudin & Anders | 2020 | 181.174 | -61.308 | 0.559 | -5.948 | -0.41 | â |
| Liu & Pang | 2019 | 181.132 | -61.303 | 0.557 | -5.957 | -0.265 | â |
| Monteiro & Dias | 2019 | 181.174 | -61.308 | â | â | â | 2.757 |
| Cantat-Gaudin et al. | 2018 | 181.174 | -61.308 | 0.559 | -5.948 | -0.41 | 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 | 1.64 | 0.87 | â | 89 | -0.158 | â | â | â |
| Almeida et al. | 2025 | 1.62 | 0.93 | â | 91 | â | 164 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 538* | â | â |
| Cavallo et al. | 2024 | 1.48 | 0.84 | â | 240 | -0.110 | â | â | â |
| Hunt & Reffert | 2023 | 1.61 | 0.63 | 0.80 | 109 | â | â | â | â |
| Almeida et al. | 2023 | 1.70 | 1.01 | â | 166 | 0.012 | 142* | 0.44 | â |
| Rain et al. | 2021 | 1.70 | 0.81 | â | 79 | â | â | â | 0 |
| Dias et al. | 2021 | 1.62 | 0.93 | â | 91 | 0.088 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.72 | 0.58 | â | 214 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.70 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 339 | 0.250 | â | â | â |
| Monteiro & Dias | 2019 | 1.68 | 0.83 | â | 81 | 0.014 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.70 | 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.