Gulliver 37

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0.80 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 102
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.75 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
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Gulliver 37 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

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

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for Gulliver 37 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 292.077 25.347 0.651 -0.772 -3.71 11.53
Hu & Soubiran 2025 292.068 25.335 – – – –
Almeida et al. 2025 292.088 25.336 – – – –
Hunt & Reffert 2024 292.074 25.358 0.648 -0.779 -3.694 9.404
Cavallo et al. 2024 292.068 25.335 0.654 – – –
Hunt & Reffert 2023 292.074 25.358 0.648 -0.779 -3.694 9.404
Almeida et al. 2023 292.075 25.331 – – – –
Tarricq et al. 2022 292.086 25.364 0.657 -0.771 -3.734 –
Dias et al. 2021 292.088 25.336 0.652 -0.767 -3.726 –
Cantat-Gaudin et al. 2020 292.077 25.347 0.642 -0.775 -3.74 –
Cantat-Gaudin & Anders 2020 292.077 25.347 0.642 -0.775 -3.74 –
Monteiro & Dias 2019 292.077 25.347 – – – 2.514
Soubiran et al. 2018 292.077 25.347 – – – 2.52
Cantat-Gaudin et al. 2018 292.077 25.347 0.642 -0.775 -3.74 –

💡 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
Hu & Soubiran 2025 – – – – -0.040* – – –
Almeida et al. 2025 1.42 1.70 – 294 – 254 – –
Hunt & Reffert 2024 – – – – – 524* – –
Cavallo et al. 2024 1.45 1.12 – 912 0.670 – – –
Hunt & Reffert 2023 1.48 1.51 0.86 262 – – – –
Almeida et al. 2023 1.48 1.89 – 182 -0.036 306* 0.58 –
Tarricq et al. 2022 1.38 – – 355 – – – –
Dias et al. 2021 1.42 1.70 – 294 0.310 – – –
Cantat-Gaudin et al. 2020 1.44 1.33 – 355 – – – –
Cantat-Gaudin & Anders 2020 1.49 – – – – – – –
Monteiro & Dias 2019 1.73 1.64 – 323 0.040 – – –
Soubiran et al. 2018 1.49 – – – – – – –
Cantat-Gaudin et al. 2018 1.49 – – – – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14062 80.4 292.08 25.35 0.65 -0.77 -3.71 11.53 0.0

💡 Note: The % column shows the percentage of members that Gulliver 37 shares with each listed object.

Visualization
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Gulliver 37 UCC
Gulliver 37 HUNT23
Gulliver 37 CANTAT20
Galactocentric position diagram