Gulliver 17
(FoF 496)
0.77
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 17 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately 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
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 302.658 | 35.868 | 0.555 | -1.085 | -3.103 | 12.637 |
| Almeida et al. | 2025 | 302.662 | 35.875 | â | â | â | â |
| Hunt & Reffert | 2024 | 302.654 | 35.867 | 0.558 | -1.094 | -3.116 | 7.178 |
| Cavallo et al. | 2024 | 302.666 | 35.873 | 0.561 | â | â | â |
| Hunt & Reffert | 2023 | 302.654 | 35.867 | 0.558 | -1.094 | -3.116 | 7.178 |
| Almeida et al. | 2023 | 302.685 | 35.87 | â | â | â | â |
| Dias et al. | 2021 | 302.662 | 35.875 | 0.557 | -1.091 | -3.028 | â |
| Cantat-Gaudin et al. | 2020 | 302.654 | 35.871 | 0.555 | -1.078 | -3.029 | â |
| Cantat-Gaudin & Anders | 2020 | 302.654 | 35.871 | 0.555 | -1.078 | -3.029 | â |
| Liu & Pang | 2019 | 302.711 | 35.845 | 0.51 | -1.661 | -4.055 | â |
| Monteiro & Dias | 2019 | 302.654 | 35.871 | â | â | â | 2.356 |
| Cantat-Gaudin et al. | 2018 | 302.654 | 35.871 | 0.555 | -1.078 | -3.029 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.58 | 1.24 | â | 55 | â | 510 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 514* | â | â |
| Cavallo et al. | 2024 | 1.76 | 1.39 | â | 63 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 1.71 | 1.10 | 1.25 | 87 | â | â | â | â |
| Almeida et al. | 2023 | 1.66 | 1.25 | â | 104 | 0.137 | 511* | 0.58 | â |
| Dias et al. | 2021 | 1.58 | 1.24 | â | 55 | 0.115 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.63 | 0.92 | â | 69 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.71 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 29 | 0.250 | â | â | â |
| Monteiro & Dias | 2019 | 1.92 | 1.26 | â | 45 | 0.029 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.71 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.