HSC 1751

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C3
N_50
r_50
DB 26 69.8
Summary

HSC 1751 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, below 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) 96.276 -13.469 2.78 -4.952 1.104 17.933
           
UCC 95.89 -13.538 2.769 -4.921 1.164 16.625
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Hunt & Reffert (2023) AV50=0.06, diffAV50=0.322, MOD50=7.69, logAge50=8.041

Search coordinates in Bayestar19

Cluster region map