HSC 1709

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C3
N_50
r_50
DC 25 68.8
Summary

HSC 1709 is a poorly populated, loose object of very low C3 quality. It is located at a very close distance from the Sun, near 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) 93.09 -8.811 4.787 -1.118 -20.898 6.917
Cavallo et al. (2024) 92.79 -8.804 4.783
           
UCC 92.739 -8.343 4.774 -0.987 -20.947 25.553
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=0.397, diffAV50=0.604, MOD50=6.659, logAge50=8.437
Cavallo et al. (2024) AV50=0.7, dMod50=6.57, logAge50=8.5, [Fe/H]50=0.33

Search coordinates in Bayestar19

Cluster region map