HSC 1710

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C3
N_50
r_50
DC 25 201.8
Summary

HSC 1710 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) 61.141 -21.449 7.264 14.348 11.841 23.013
Cavallo et al. (2024) 62.566 -23.457 7.182
           
UCC 62.647 -23.513 7.153 15.631 11.338 26.942
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
Hunt & Reffert (2023) AV50=0.074, diffAV50=0.335, MOD50=5.638, logAge50=8.097
Cavallo et al. (2024) AV50=0.62, dMod50=5.76, logAge50=7.89, [Fe/H]50=0.28

Search coordinates in Bayestar19

Cluster region map