Gulliver 13
(CMa03)
0.82
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
8.2 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 13 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 104.858 | -13.256 | 0.626 | -2.935 | 0.294 | 57.842 |
| Li et al. | 2025 | 104.858 | -13.254 | 0.62 | -2.941 | 0.281 | â |
| Hu & Soubiran | 2025 | 104.869 | -13.242 | â | â | â | â |
| Almeida et al. | 2025 | 104.874 | -13.247 | â | â | â | â |
| Hunt & Reffert | 2024 | 104.877 | -13.249 | 0.617 | -2.941 | 0.302 | 52.009 |
| Cavallo et al. | 2024 | 104.869 | -13.242 | 0.622 | â | â | â |
| Hunt & Reffert | 2023 | 104.877 | -13.249 | 0.617 | -2.941 | 0.302 | 52.009 |
| Almeida et al. | 2023 | 104.877 | -13.237 | â | â | â | â |
| Tarricq et al. | 2022 | 104.852 | -13.249 | 0.623 | -2.919 | 0.296 | â |
| Santos-Silva et al. | 2021 | 104.86 | -13.25 | 0.63 | -2.92 | 0.31 | â |
| Dias et al. | 2021 | 104.874 | -13.247 | 0.617 | -2.935 | 0.301 | 56.889 |
| Cantat-Gaudin et al. | 2020 | 104.858 | -13.254 | 0.62 | -2.941 | 0.281 | â |
| Cantat-Gaudin & Anders | 2020 | 104.858 | -13.254 | 0.62 | -2.941 | 0.281 | â |
| Monteiro & Dias | 2019 | 104.858 | -13.254 | â | â | â | 2.534 |
| Soubiran et al. | 2018 | 104.858 | -13.254 | â | â | â | 56.53 |
| Cantat-Gaudin et al. | 2018 | 104.858 | -13.254 | 0.62 | -2.941 | 0.281 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.5 | 1.33 | 2.23 | 626 | -0.050 | 351 | 0.53 | â |
| Li et al. | 2025 | 1.46 | 0.91 | â | 1056 | -0.036 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.140(5) | â | â | â |
| Almeida et al. | 2025 | 1.50 | 1.68 | â | 594 | â | 351 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 395(1) | â | â |
| Cavallo et al. | 2024 | 1.39 | 1.09 | â | 1047 | 0.000 | â | â | â |
| Hunt & Reffert | 2023 | 1.48 | 1.33 | 2.23 | 600 | â | â | â | â |
| Almeida et al. | 2023 | 1.47 | 1.58 | â | 653 | -0.115 | 351(1) | 0.53 | â |
| Tarricq et al. | 2022 | 1.47 | â | â | 1072 | â | â | â | â |
| Santos-Silva et al. | 2021 | 1.53(1) | 1.71(1) | â | 536(1) | -0.120(1) | â | â | â |
| Dias et al. | 2021 | 1.50 | 1.68 | â | 594 | -0.050 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.51 | 0.78 | â | 1000 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.54 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.66 | 1.26 | â | 33 | 0.031 | â | â | â |
| Soubiran et al. | 2018 | 1.54 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.54 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.