Gulliver 15
0.75
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
5.9 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 15 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, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
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 | 272.594 | -16.722 | 0.519 | -1.032 | -1.645 | -13.388 |
| Hu & Soubiran | 2025 | 272.594 | -16.71 | â | â | â | â |
| Almeida et al. | 2025 | 272.603 | -16.715 | â | â | â | â |
| Hunt & Reffert | 2024 | 272.598 | -16.723 | 0.497 | -1.014 | -1.658 | 12.34 |
| Cavallo et al. | 2024 | 272.594 | -16.71 | 0.502 | â | â | â |
| Hunt & Reffert | 2023 | 272.598 | -16.723 | 0.497 | -1.014 | -1.658 | 12.34 |
| Dias et al. | 2021 | 272.603 | -16.715 | 0.484 | -1.071 | -1.621 | â |
| Cantat-Gaudin et al. | 2020 | 272.599 | -16.723 | 0.506 | -1.06 | -1.638 | â |
| Cantat-Gaudin & Anders | 2020 | 272.599 | -16.723 | 0.506 | -1.06 | -1.638 | â |
| Monteiro & Dias | 2019 | 272.599 | -16.723 | â | â | â | 2.276 |
| Cantat-Gaudin et al. | 2018 | 272.599 | -16.723 | 0.506 | -1.06 | -1.638 | 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 | -0.240* | â | â | â |
| Almeida et al. | 2025 | 1.88 | 2.49 | â | 12 | â | 574 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1110* | â | â |
| Cavallo et al. | 2024 | 1.49 | 2.70 | â | 537 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 1.78 | 2.79 | 2.66 | 93 | â | â | â | â |
| Dias et al. | 2021 | 1.88 | 2.49 | â | 12 | -0.044 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.04 | 2.08 | â | 85 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.87 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.71 | 2.66 | â | 24 | 0.007 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.87 | 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.