Gulliver 24

(FoF 2126)

Click to load Aladin Lite
0.80 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 129
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
Gulliver 24 is a rich, very dense object of 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, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Intermediate age

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

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for Gulliver 24 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 1.141 62.836 0.654 -3.218 -1.564 -32.7
Almeida et al. 2025 1.169 62.843 – – – –
Hunt & Reffert 2024 1.14 62.836 0.653 -3.204 -1.568 -36.737
Cavallo et al. 2024 1.135 62.847 0.655 – – –
Hunt & Reffert 2023 1.14 62.836 0.653 -3.204 -1.568 -36.737
Almeida et al. 2023 1.134 62.837 – – – –
Tarricq et al. 2022 1.121 62.824 0.662 -3.226 -1.58 –
Dias et al. 2021 1.169 62.843 0.641 -3.254 -1.562 –
Cantat-Gaudin et al. 2020 1.161 62.835 0.636 -3.241 -1.57 –
Cantat-Gaudin & Anders 2020 1.161 62.835 0.636 -3.241 -1.57 –
Liu & Pang 2019 1.148 62.827 0.639 -3.185 -1.48 –
Monteiro & Dias 2019 1.161 62.835 – – – 3.538
Soubiran et al. 2018 1.161 62.835 – – – -31.86
Cantat-Gaudin et al. 2018 1.161 62.835 0.636 -3.241 -1.57 –

💡 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 1.42 1.37 – 248 – 239 – –
Hunt & Reffert 2024 – – – – – 509* – –
Cavallo et al. 2024 1.61 1.39 – 316 0.420 – – –
Hunt & Reffert 2023 1.44 1.48 1.42 126 – – – –
Almeida et al. 2023 1.42 1.51 – 185 0.005 218* 0.51 –
Tarricq et al. 2022 1.44 – – 191 – – – –
Dias et al. 2021 1.42 1.37 – 248 0.103 – – –
Cantat-Gaudin et al. 2020 1.50 1.05 – 178 – – – –
Cantat-Gaudin & Anders 2020 1.50 – – – – – – –
Liu & Pang 2019 – – – 209 -0.250 – – –
Monteiro & Dias 2019 1.49 0.95 – 126 0.016 – – –
Soubiran et al. 2018 1.50 – – – – – – –
Cantat-Gaudin et al. 2018 1.50 – – – – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10420 58.9 1.15 62.83 0.66 -3.21 -1.56 -32.67 0.0

💡 Note: The % column shows the percentage of members that Gulliver 24 shares with each listed object.

Visualization
ℹī¸
Gulliver 24 UCC
Gulliver 24 HUNT23
Gulliver 24 CANTAT20
Galactocentric position diagram