Gulliver 38
(FoF 1747)
0.79
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 38 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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
Massive
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 | 300.809 | 34.437 | 0.407 | -0.918 | -2.584 | 10.227 |
| Hu & Soubiran | 2025 | 300.817 | 34.441 | â | â | â | â |
| Hunt & Reffert | 2024 | 300.805 | 34.435 | 0.4 | -0.906 | -2.616 | 5.581 |
| Cavallo et al. | 2024 | 300.816 | 34.441 | 0.401 | â | â | â |
| Hunt & Reffert | 2023 | 300.805 | 34.435 | 0.4 | -0.906 | -2.616 | 5.581 |
| Cantat-Gaudin et al. | 2020 | 300.808 | 34.435 | 0.4 | -0.921 | -2.594 | â |
| Cantat-Gaudin & Anders | 2020 | 300.808 | 34.435 | 0.4 | -0.921 | -2.594 | â |
| Liu & Pang | 2019 | 300.812 | 34.44 | 0.397 | -0.925 | -2.635 | â |
| Monteiro & Dias | 2019 | 300.808 | 34.435 | â | â | â | 3.474 |
| Soubiran et al. | 2018 | 300.808 | 34.435 | â | â | â | 10.62 |
| Cantat-Gaudin et al. | 2018 | 300.808 | 34.435 | 0.4 | -0.921 | -2.594 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.140* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1436* | â | â |
| Cavallo et al. | 2024 | 2.37 | 2.50 | â | 525 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 2.31 | 2.24 | 2.23 | 385 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.44 | 1.64 | â | 813 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.33 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 851 | 0.250 | â | â | â |
| Monteiro & Dias | 2019 | 3.24 | 1.94 | â | 14 | 0.010 | â | â | â |
| Soubiran et al. | 2018 | 2.33 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.33 | 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)
Gold sample.