Gulliver 11
Summary
Gulliver 11 is a moderately populated, very dense object of high C3 quality. It is located at a close distance from the Sun, near the mid-plane. It is well-studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Cantat-Gaudin et al. (2018) | 67.996 | 43.62 | 1.061 | 0.4 | -2.229 | – |
| Cantat-Gaudin et al. (2020) | 67.996 | 43.62 | 1.061 | 0.4 | -2.229 | – |
| Dias et al. (2021) | 68.016 | 43.602 | 1.068 | 0.399 | -2.221 | – |
| Tarricq et al. (2022) | 67.971 | 43.66 | 1.046 | 0.274 | -2.355 | – |
| Hunt & Reffert (2023) | 68.009 | 43.613 | 1.071 | 0.318 | -2.282 | 1.277 |
| Cavallo et al. (2024) | 68.025 | 43.623 | 1.07 | – | – | – |
| Hunt & Reffert (2024) | 68.009 | 43.613 | 1.071 | 0.318 | -2.282 | 1.277 |
| Alfonso et al. (2024) | 68.003 | 43.619 | 1.031 | 0.304 | -2.303 | – |
| Almeida et al. (2025) | 68.016 | 43.602 | – | – | – | – |
| UCC | 68.027 | 43.621 | 1.06 | 0.323 | -2.279 | -3.46 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Cantat-Gaudin et al. (2018) | dmode=917.3 |
| Cantat-Gaudin et al. (2020) | AVNN=0.76, DistPc=907.0, AgeNN=8.51 |
| Dias et al. (2021) | Av=1.526, Dist=925, logage=8.535, [Fe/H]=-0.09 |
| Tarricq et al. (2022) | Dist=885, logAgeNN=8.52 |
| Hunt & Reffert (2023) | AV50=1.19, diffAV50=1.09, MOD50=9.785, logAge50=8.326 |
| Cavallo et al. (2024) | AV50=1.15, dMod50=9.85, logAge50=8.55, [Fe/H]50=0.34 |
| Hunt & Reffert (2024) | MassJ=179.001, MassTot=222.926 |
| Alfonso et al. (2024) | AV=0.76152, MOD=9.75532, logAge=8.52299, Z=-0.0885 |
| Almeida et al. (2025) | AV=1.526, Dist=925, logAge=8.535, MassRk=157.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 14370 | 80.3 | 68.03 | 43.62 | 1.08 | 0.29 | -2.28 | -3.46 | 0.0 |
