HSC 2395

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C3
N_50
r_50
BB 21 3.0
Summary

HSC 2395 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a significant 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) 165.537 -59.998 0.194 -7.243 2.915 -2.264
Cavallo et al. (2024) 165.743 -59.976 0.193
Hunt & Reffert (2024) 165.537 -59.998 0.194 -7.243 2.915 -2.264
           
UCC 165.555 -59.999 0.187 -7.163 2.923
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=1.912, diffAV50=2.518, MOD50=13.332, logAge50=7.748
Cavallo et al. (2024) AV50=1.93, dMod50=13.33, logAge50=7.96, [Fe/H]50=0.65
Hunt & Reffert (2024) MassJ=513.106, MassTot=1023.95

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3283 60.0 165.57 -60.0 0.19 -7.14 2.96 -32.64 0.07