Gulliver 48
0.77
UTI
0.72
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
12.3 [arcmin]
- CN 0.72 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 48 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
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 | 316.351 | 50.746 | 1.066 | -4.784 | -6.718 | -18.355 |
| Li et al. | 2025 | 316.334 | 50.733 | 1.058 | -4.781 | -6.671 | â |
| Alfonso et al. | 2024 | 316.513 | 50.69 | 1.038 | -4.769 | -6.656 | â |
| Hunt & Reffert | 2024 | 316.304 | 50.741 | 1.056 | -4.772 | -6.699 | -4.923 |
| Celli et al. | 2024 | 316.334 | 50.733 | â | â | â | â |
| Cavallo et al. | 2024 | 316.329 | 50.725 | 1.066 | â | â | â |
| Hunt & Reffert | 2023 | 316.304 | 50.741 | 1.056 | -4.772 | -6.699 | -4.923 |
| He et al. | 2022 | 316.303 | 50.737 | 1.069 | -4.778 | -6.717 | â |
| Cantat-Gaudin et al. | 2020 | 316.334 | 50.733 | 1.058 | -4.781 | -6.671 | â |
| Cantat-Gaudin & Anders | 2020 | 316.334 | 50.733 | 1.058 | -4.781 | -6.671 | â |
| Monteiro & Dias | 2019 | 316.334 | 50.733 | â | â | â | 2.624 |
| Soubiran et al. | 2018 | 316.334 | 50.733 | â | â | â | -26.67 |
| Cantat-Gaudin et al. | 2018 | 316.334 | 50.733 | 1.058 | -4.781 | -6.671 | 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 | 0.67 | 2.68 | â | 212 | 0.037 | â | â | â |
| Alfonso et al. | 2024 | 1.04 | 2.87 | â | 41 | 0.010 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 597* | â | â |
| Celli et al. | 2024 | â | â | â | 18 | â | 640 | â | â |
| Cavallo et al. | 2024 | 1.24 | 3.32 | â | 32 | 0.690 | â | â | â |
| Hunt & Reffert | 2023 | 0.90 | 3.40 | 2.79 | 38 | â | â | â | â |
| He et al. | 2022 | â | 3.40 | â | 20 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.04 | 2.87 | â | 18 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.92 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.89 | 2.40 | â | 210 | 0.015 | â | â | â |
| Soubiran et al. | 2018 | 0.92 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.92 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.