HSC 2409

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C3
N_50
r_50
BC 16 3.4
Summary

HSC 2409 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

This object shares a small 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) 163.541 -65.671 0.138 -5.584 2.499 51.174
Hunt & Reffert (2024) 163.541 -65.671 0.138 -5.584 2.499 51.174
           
UCC 163.544 -65.659 0.139 -5.56 2.483 51.293
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=1.348, diffAV50=1.249, MOD50=13.937, logAge50=9.633
Hunt & Reffert (2024) MassJ=942.026, MassTot=1383.68

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4861 12.0 163.36 -65.54 0.18 -5.83 2.42 24.13 0.03