HXWHB 7

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C3
N_50
r_50
DC 14 10.9
Summary

HXWHB 7 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature.

This is likely a unique object, which shares a moderate percentage of members with at least one previously 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=0.64) 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) 80.57 35.42 0.58 1.49 -2.88
           
UCC 80.64 35.32 0.55 1.542 -2.872 5.901
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

HXWHB 7 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Hao et al. (2020) AG=1.18, d_pc=1735.0, logt=7.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 26 36.0 80.68 35.27 0.38 1.85 -2.86 14.27 0.67