DBSB 66

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C3
N_50
r_50
DC 40 7.6
Summary

DBSB 66 is a poorly populated, very loose object of very 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: 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) 169.11 -61.485 -11.49 2.16
           
UCC 169.201 -61.463 0.311 -7.59 2.222 -14.393
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

DBSB 66 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=0.999, distance=7511, log_age=6.0

Search coordinates in Bayestar19

Cluster region map