HSC 2151

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C3
N_50
r_50
BB 21 2.3
Summary

HSC 2151 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

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) 131.178 -47.689 0.118 -3.125 3.481 75.19
Cavallo et al. (2024) 131.166 -47.67 0.119
Hunt & Reffert (2024) 131.178 -47.689 0.118 -3.125 3.481 75.19
           
UCC 131.175 -47.689 0.118 -3.142 3.479 75.33
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=2.021, diffAV50=0.877, MOD50=14.178, logAge50=7.537
Cavallo et al. (2024) AV50=1.35, dMod50=13.59, logAge50=8.51, [Fe/H]50=0.37
Hunt & Reffert (2024) MassJ=566.006, MassTot=566.006

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3947 88.0 131.18 -47.68 0.12 -3.15 3.48 75.33 0.02