HSC 2251

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C3
N_50
r_50
BB 29 61.1
Summary

HSC 2251 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.79) 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) 154.881 -45.523 2.429 -0.591 -0.173 -8.222
Cavallo et al. (2024) 151.251 -44.276 2.432
           
UCC 151.208 -44.023 2.441 -0.694 -0.108 -8.052
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=0.086, diffAV50=0.287, MOD50=7.925, logAge50=8.728
Cavallo et al. (2024) AV50=0.34, dMod50=8.09, logAge50=8.35, [Fe/H]50=0.05

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1161 20.7 154.49 -45.44 2.53 -0.27 -0.55 -9.07 0.07