Gulliver 10
0.85
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
12.8 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 10 is a rich, very dense object of very high 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, very young cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is well-studied in the literature.
Close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 123.107 | -38.647 | 1.667 | -4.39 | 5.052 | 25.37 |
| Almeida et al. | 2025 | 123.024 | -38.659 | â | â | â | â |
| Alfonso et al. | 2024 | 124.148 | -38.718 | 1.612 | -4.947 | 5.21 | â |
| Hunt & Reffert | 2024 | 123.134 | -38.712 | 1.684 | -4.364 | 5.09 | 27.621 |
| Celli et al. | 2024 | 123.09 | -38.676 | â | â | â | â |
| Cavallo et al. | 2024 | 123.168 | -38.687 | 1.682 | â | â | â |
| Hunt & Reffert | 2023 | 123.134 | -38.712 | 1.684 | -4.364 | 5.09 | 27.621 |
| He et al. | 2022 | 123.153 | -38.675 | 1.695 | -4.321 | 5.076 | â |
| Dias et al. | 2021 | 123.024 | -38.659 | 1.661 | -4.428 | 4.948 | 33.422 |
| Cantat-Gaudin et al. | 2020 | 123.09 | -38.676 | 1.652 | -4.443 | 4.965 | â |
| Cantat-Gaudin & Anders | 2020 | 123.09 | -38.676 | 1.652 | -4.443 | 4.965 | â |
| Monteiro & Dias | 2019 | 123.09 | -38.676 | â | â | â | 2.154 |
| Soubiran et al. | 2018 | 123.09 | -38.676 | â | â | â | 32.64 |
| Cantat-Gaudin et al. | 2018 | 123.09 | -38.676 | 1.652 | -4.443 | 4.965 | 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 | 0.52 | 0.34 | â | 13 | â | 57 | â | â |
| Alfonso et al. | 2024 | 0.61 | 0.62 | â | 11 | 0.134 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 89* | â | â |
| Celli et al. | 2024 | â | â | â | 9 | â | 79 | â | â |
| Cavallo et al. | 2024 | 0.86 | 1.87 | â | 309 | 0.710 | â | â | â |
| Hunt & Reffert | 2023 | 0.57 | 2.25 | 2.12 | 5 | â | â | â | â |
| He et al. | 2022 | â | 2.00 | â | 6 | â | â | â | â |
| Dias et al. | 2021 | 0.52 | 0.34 | â | 13 | 0.134 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.61 | 0.62 | â | 9 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.59 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.57 | 1.88 | â | 7 | 0.006 | â | â | â |
| Soubiran et al. | 2018 | 0.59 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.59 | 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.
Cavallo et al. (2024)
Wood sample.