DBSB 167

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C3
N_50
r_50
CC 17 4.4
Summary

DBSB 167 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.

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
Kharchenko et al. (2012) 245.857 -49.545 -5.61 2.95
           
UCC 245.77 -49.475 0.271 -3.758 -3.65 -47.864
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

DBSB 167 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=1.395, distance=4076, log_age=6.2

Search coordinates in Bayestar19

Cluster region map