Gulliver 11

Click to load Aladin Lite
0.80 UTI
0.6
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
N50 (P>50% members) 71
Stellar density (N50/rad) 19.8 [N/pc2]
C3 classification AB
  • CN 0.6 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.81 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
Gulliver 11 is a moderately populated, very dense object of 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, intermediate-age 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.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Liu et al. (2025)
Classified as primordial binary cluster 158 along with HSC_1256, and as hyperbolic encounter pair 277 along with NGC_1582, and of multiple system 24 along with CWNU_361, NGC_1582 and HSC_1256.

Palma et al. (2025)
Part of multiple system G92, along with NGC_1582, CWNU_361 and HSC_1256.

Cavallo et al. (2024)
Gold sample.

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

Data
🔍 Search references for Gulliver 11 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 68.027 43.621 1.06 0.323 -2.279 -3.46
Liu et al. 2025 68.01 43.61 1.07 0.32 -2.28 1.28
Li et al. 2025 67.996 43.62 1.061 0.4 -2.229 –
Almeida et al. 2025 68.016 43.602 – – – –
Alfonso et al. 2024 68.003 43.619 1.031 0.304 -2.303 –
Zhang et al. 2024 68.009 43.613 – – – –
Hunt & Reffert 2024 68.009 43.613 1.071 0.318 -2.282 1.277
Cavallo et al. 2024 68.025 43.623 1.07 – – –
Hunt & Reffert 2023 68.009 43.613 1.071 0.318 -2.282 1.277
Almeida et al. 2023 68.028 43.612 – – – –
Tarricq et al. 2022 67.971 43.66 1.046 0.274 -2.355 –
Dias et al. 2021 68.016 43.602 1.068 0.399 -2.221 –
Cantat-Gaudin et al. 2020 67.996 43.62 1.061 0.4 -2.229 –
Zhong et al. 2020 67.996 43.62 – 0.4 -2.229 -3.692
Cantat-Gaudin & Anders 2020 67.996 43.62 1.061 0.4 -2.229 –
Monteiro & Dias 2019 67.996 43.62 – – – 2.455
Cantat-Gaudin et al. 2018 67.996 43.62 1.061 0.4 -2.229 –

💡 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 99999– 0.915 1.15 1.09 328 -0.033 158 0.52 –
Liu et al. 2025 1.51 0.42 – 72 – – – –
Li et al. 2025 0.83 0.96 – 351 -0.065 – – –
Almeida et al. 2025 0.93 1.53 – 343 – 158 – –
Alfonso et al. 2024 0.89 0.76 – 333 -0.088 – – –
Zhang et al. 2024 – – – – -0.240(1) – – –
Hunt & Reffert 2024 – – – – – 179(1) – –
Cavallo et al. 2024 0.93 1.15 – 355 0.340 – – –
Hunt & Reffert 2023 0.91 1.19 1.09 212 – – – –
Almeida et al. 2023 0.90 1.35 – 219 -0.001 106(1) 0.52 –
Tarricq et al. 2022 0.89 – – 331 – – – –
Dias et al. 2021 0.93 1.53 – 343 -0.090 – – –
Cantat-Gaudin et al. 2020 0.91 0.76 – 324 – – – –
Zhong et al. 2020 0.00 0.00 – 0 0.021 – – –
Cantat-Gaudin & Anders 2020 0.92 – – – – – – –
Monteiro & Dias 2019 1.06 1.22 – 303 0.026 – – –
Cantat-Gaudin et al. 2018 0.92 – – – – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

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

💡 Note: The % column shows the percentage of members that Gulliver 11 shares with each listed object.

Visualization
ℹī¸
Gulliver 11 UCC
Gulliver 11 HUNT23
Gulliver 11 CANTAT20
Galactocentric position diagram