HXWHB 5

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C3
N_50
r_50
AC 16 12.1
Summary

HXWHB 5 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature.

Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.32) 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
Hao et al. (2020) 80.37 33.39 0.79 -0.12 -3.18
           
UCC 80.507 33.558 0.86 -0.245 -3.125 51.539
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

HXWHB 5 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Hao et al. (2020) AG=0.88, d_pc=1266.8, logt=7.74

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 8 68.0 80.56 33.79 0.9 -0.3 -3.07 6.27 0.21
Teutsch 89 60.0 80.56 33.77 0.9 -0.35 -3.12 -6.34 0.46
HXWHB 8 40.0 80.56 33.78 0.91 -0.31 -3.1 -3.92 0.0