Gulliver 14

Click to load Aladin Lite
0.83 UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.79
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 65
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.79 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
Gulliver 14 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near 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.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for Gulliver 14 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 259.925 -36.742 0.763 -3.761 -4.79 -15.558
Li et al. 2025 259.928 -36.785 0.745 -3.719 -4.792 –
Hu & Soubiran 2025 259.928 -36.738 – – – –
Almeida et al. 2025 259.915 -36.763 – – – –
Hunt & Reffert 2024 259.946 -36.708 0.763 -3.759 -4.756 -16.263
Cavallo et al. 2024 259.928 -36.738 0.76 – – –
Hunt & Reffert 2023 259.946 -36.708 0.763 -3.759 -4.756 -16.263
Almeida et al. 2023 259.899 -36.805 – – – –
Tarricq et al. 2022 259.956 -36.702 0.748 -3.751 -4.795 –
Dias et al. 2021 259.915 -36.763 0.741 -3.733 -4.779 –
Cantat-Gaudin et al. 2020 259.928 -36.785 0.745 -3.719 -4.792 –
Cantat-Gaudin & Anders 2020 259.928 -36.785 0.745 -3.719 -4.792 –
Monteiro & Dias 2019 259.928 -36.785 – – – 2.4
Soubiran et al. 2018 259.928 -36.785 – – – -13.36
Cantat-Gaudin et al. 2018 259.928 -36.785 0.745 -3.719 -4.792 –

💡 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
Li et al. 2025 1.01 1.68 – 709 -0.048 – – –
Hu & Soubiran 2025 – – – – -0.080* – – –
Almeida et al. 2025 1.26 2.00 – 343 – 173 – –
Hunt & Reffert 2024 – – – – – 316* – –
Cavallo et al. 2024 1.14 1.81 – 832 0.090 – – –
Hunt & Reffert 2023 1.24 1.93 0.99 394 – – – –
Almeida et al. 2023 1.19 1.87 – 470 0.201 170* 0.57 –
Tarricq et al. 2022 1.20 – – 661 – – – –
Dias et al. 2021 1.26 2.00 – 343 0.170 – – –
Cantat-Gaudin et al. 2020 1.25 1.63 – 603 – – – –
Cantat-Gaudin & Anders 2020 1.29 – – – – – – –
Monteiro & Dias 2019 1.19 1.48 – 673 0.026 – – –
Soubiran et al. 2018 1.29 – – – – – – –
Cantat-Gaudin et al. 2018 1.29 – – – – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization
ℹī¸
Gulliver 14 UCC
Gulliver 14 HUNT23
Gulliver 14 CANTAT20
Galactocentric position diagram