HSC 2477

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C3
N_50
r_50
CB 17 3.5
Summary

HSC 2477 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

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) 180.142 -62.863 0.217 -6.41 0.947 18.717
Cavallo et al. (2024) 180.155 -62.863 0.219
Hunt & Reffert (2024) 180.142 -62.863 0.217 -6.41 0.947 18.717
           
UCC 180.154 -62.848 0.215 -6.409 0.94 3.35
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=3.226, diffAV50=2.249, MOD50=13.076, logAge50=8.672
Cavallo et al. (2024) AV50=2.88, dMod50=12.83, logAge50=8.93, [Fe/H]50=-0.56
Hunt & Reffert (2024) MassJ=554.466, MassTot=736.744

Search coordinates in Bayestar19

Cluster region map