HSC 1714

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C3
N_50
r_50
DC 26 178.8
Summary

HSC 1714 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Hunt & Reffert (2023) 77.721 -16.006 4.683 -10.224 -1.504 20.128
Cavallo et al. (2024) 79.784 -13.955 4.681
           
UCC 79.576 -13.764 4.645 -10.215 -1.857 21.352
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
Hunt & Reffert (2023) AV50=0.048, diffAV50=0.332, MOD50=6.645, logAge50=8.215
Cavallo et al. (2024) AV50=0.33, dMod50=6.71, logAge50=8.18, [Fe/H]50=0.33

Search coordinates in Bayestar19

Cluster region map