Gulliver 28
0.58
UTI
0.3
CN
0.51
Cdens
0.5
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
18.6 [arcmin]
- CN 0.3 Poorly populated
- Cdens 0.51 Moderately dense
- CC3 0.5 Intermediate quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 28 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Close
Moderate 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 | 293.531 | 18.072 | 1.579 | -4.453 | -3.472 | 3.984 |
| Li et al. | 2025 | 293.559 | 18.059 | 1.581 | -4.485 | -3.4 | â |
| Almeida et al. | 2025 | 293.612 | 18.039 | â | â | â | â |
| Alfonso et al. | 2024 | 293.483 | 17.993 | 1.54 | -4.445 | -3.478 | â |
| Hunt & Reffert | 2024 | 293.654 | 18.164 | 1.542 | -4.419 | -3.472 | 3.062 |
| Cavallo et al. | 2024 | 293.483 | 18.27 | 1.549 | â | â | â |
| Hunt & Reffert | 2023 | 293.654 | 18.164 | 1.542 | -4.419 | -3.472 | 3.062 |
| Almeida et al. | 2023 | 293.924 | 18.053 | â | â | â | â |
| Tarricq et al. | 2022 | 293.396 | 18.082 | 1.593 | -4.43 | -3.477 | â |
| Dias et al. | 2021 | 293.612 | 18.039 | 1.568 | -4.468 | -3.384 | 1.823 |
| Cantat-Gaudin et al. | 2020 | 293.559 | 18.059 | 1.581 | -4.485 | -3.4 | â |
| Cantat-Gaudin & Anders | 2020 | 293.559 | 18.059 | 1.581 | -4.485 | -3.4 | â |
| Monteiro & Dias | 2019 | 293.559 | 18.059 | â | â | â | 2.299 |
| Soubiran et al. | 2018 | 293.559 | 18.059 | â | â | â | 0.97 |
| Cantat-Gaudin et al. | 2018 | 293.559 | 18.059 | 1.581 | -4.485 | -3.4 | 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 | 0.51 | 1.13 | â | 1046 | -0.052 | â | â | â |
| Almeida et al. | 2025 | 0.59 | 1.14 | â | 906 | â | 132 | â | â |
| Alfonso et al. | 2024 | 0.63 | 0.97 | â | 1154 | 0.152 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 111* | â | â |
| Cavallo et al. | 2024 | 0.65 | 1.31 | â | 282 | 0.650 | â | â | â |
| Hunt & Reffert | 2023 | 0.61 | 2.13 | 2.33 | 66 | â | â | â | â |
| Almeida et al. | 2023 | 0.50 | 1.30 | â | 1002 | -0.229 | 180* | 0.67 | â |
| Tarricq et al. | 2022 | 0.62 | â | â | 363 | â | â | â | â |
| Dias et al. | 2021 | 0.59 | 1.14 | â | 906 | 0.152 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.63 | 0.97 | â | 339 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.62 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.59 | 1.60 | â | 516 | 0.023 | â | â | â |
| Soubiran et al. | 2018 | 0.62 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.62 | 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: intermediate fit.
Cavallo et al. (2024)
Gold sample.