NGC 1724

(OCL 405; MWSC 459)

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C3
N_50
r_50
AB 25 2.5
Summary

NGC 1724 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is moderately studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Cantat-Gaudin et al. (2018) 75.838 49.495 0.244 1.02 0.048
Bica et al. (2019) 75.89 49.495
Cantat-Gaudin et al. (2020) 75.838 49.495 0.244 1.02 0.048
Dias et al. (2021) 75.847 49.498 0.243 1.045 0.057
Hunt & Reffert (2023) 75.828 49.505 0.246 0.851 -0.0
Cavallo et al. (2024) 75.861 49.512 0.246
Hunt & Reffert (2024) 75.828 49.505 0.246 0.851 -0.0
Almeida et al. (2025) 75.847 49.498
           
UCC 75.837 49.508 0.238 0.892 0.044
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Cantat-Gaudin et al. (2018) dmode=3669.0
Cantat-Gaudin et al. (2020) AVNN=1.16, DistPc=3795.0, AgeNN=8.48
Dias et al. (2021) Av=1.923, Dist=3359, logage=7.964, [Fe/H]=-0.322
Hunt & Reffert (2023) AV50=1.808, diffAV50=1.87, MOD50=12.909, logAge50=8.328
Cavallo et al. (2024) AV50=1.35, dMod50=12.85, logAge50=8.56, [Fe/H]50=0.22
Hunt & Reffert (2024) MassJ=271.602, MassTot=380.087
Almeida et al. (2025) AV=1.923, Dist=3359, logAge=7.964, MassRk=256.9

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Cluster region map