HSC 1077

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C3
N_50
r_50
DC 26 285.7
Summary

HSC 1077 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, above 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) 179.221 64.358 10.523 -69.191 -10.867 -3.663
Cavallo et al. (2024) 174.578 63.959 10.577
Hu & Soubiran (2025) 174.578 63.959
           
UCC 178.238 64.164 10.124 -69.376 -10.676 -0.961
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=0.618, diffAV50=0.442, MOD50=4.933, logAge50=9.584
Cavallo et al. (2024) AV50=0.79, dMod50=4.97, logAge50=9.25, [Fe/H]50=0.25
Hu & Soubiran (2025) MA23f=-0.49

Search coordinates in Bayestar19

Cluster region map