Gulliver 38

(FoF 1747)

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0.79 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.6 Moderately studied
  • Cdup 1.0 Unique

Overview

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Gulliver 38 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately 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 Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 300.809 34.437 0.407 -0.918 -2.584 10.227
Hu & Soubiran 2025 300.817 34.441 – – – –
Hunt & Reffert 2024 300.805 34.435 0.4 -0.906 -2.616 5.581
Cavallo et al. 2024 300.816 34.441 0.401 – – –
Hunt & Reffert 2023 300.805 34.435 0.4 -0.906 -2.616 5.581
Cantat-Gaudin et al. 2020 300.808 34.435 0.4 -0.921 -2.594 –
Cantat-Gaudin & Anders 2020 300.808 34.435 0.4 -0.921 -2.594 –
Liu & Pang 2019 300.812 34.44 0.397 -0.925 -2.635 –
Monteiro & Dias 2019 300.808 34.435 – – – 3.474
Soubiran et al. 2018 300.808 34.435 – – – 10.62
Cantat-Gaudin et al. 2018 300.808 34.435 0.4 -0.921 -2.594 –

💡 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 – – – – -0.140* – – –
Hunt & Reffert 2024 – – – – – 1436* – –
Cavallo et al. 2024 2.37 2.50 – 525 0.240 – – –
Hunt & Reffert 2023 2.31 2.24 2.23 385 – – – –
Cantat-Gaudin et al. 2020 2.44 1.64 – 813 – – – –
Cantat-Gaudin & Anders 2020 2.33 – – – – – – –
Liu & Pang 2019 – – – 851 0.250 – – –
Monteiro & Dias 2019 3.24 1.94 – 14 0.010 – – –
Soubiran et al. 2018 2.33 – – – – – – –
Cantat-Gaudin et al. 2018 2.33 – – – – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2844 89.0 300.81 34.44 0.41 -0.92 -2.59 10.23 0.0

💡 Note: The % column shows the percentage of members that Gulliver 38 shares with each listed object.

Visualization

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